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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Mar. Sci.</journal-id>
<journal-title-group>
<journal-title>Frontiers in Marine Science</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Mar. Sci.</abbrev-journal-title>
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<issn pub-type="epub">2296-7745</issn>
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<publisher-name>Frontiers Media S.A.</publisher-name>
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<article-meta>
<article-id pub-id-type="doi">10.3389/fmars.2025.1642772</article-id>
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<article-categories>
<subj-group subj-group-type="heading">
<subject>Original Research</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>Preliminary analysis and applications of the Indian Ocean wave drifter program</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Remya</surname><given-names>P. G.</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="corresp" rid="c001"><sup>*</sup></xref>
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<name><surname>Suresh Kumar</surname><given-names>N.</given-names></name>
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<name><surname>Mithun</surname><given-names>Sundhar B.</given-names></name>
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<name><surname>Praveen Kumar</surname><given-names>B.</given-names></name>
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<name><surname>Anoop</surname><given-names>T. R.</given-names></name>
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<name><surname>Reddem</surname><given-names>Venkat Shesu</given-names></name>
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<name><surname>Jeyakumar</surname><given-names>C.</given-names></name>
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<name><surname>Lotliker</surname><given-names>Aneesh A.</given-names></name>
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<name><surname>Rao</surname><given-names>E. Pattabhi Rama</given-names></name>
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<name><surname>Nair</surname><given-names>T. M. Balakrishnan</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
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<aff id="aff1"><label>1</label><institution>Indian National Centre for Ocean Information Services, Ministry of Earth Science (MoES)</institution>, <city>Hyderabad</city>, <country country="in">India</country></aff>
<aff id="aff2"><label>2</label><institution>National Centre for Polar and Ocean Research (NCPOR)</institution>, <city>Goa</city>, <country country="in">India</country></aff>
<author-notes>
<corresp id="c001"><label>*</label>Correspondence: P. G. Remya, <email xlink:href="mailto:remya.pg@incois.gov.in">remya.pg@incois.gov.in</email></corresp>
</author-notes>
<pub-date publication-format="electronic" date-type="pub" iso-8601-date="2025-10-30">
<day>30</day>
<month>10</month>
<year>2025</year>
</pub-date>
<pub-date publication-format="electronic" date-type="collection">
<year>2025</year>
</pub-date>
<volume>12</volume>
<elocation-id>1642772</elocation-id>
<history>
<date date-type="received">
<day>07</day>
<month>06</month>
<year>2025</year>
</date>
<date date-type="accepted">
<day>03</day>
<month>10</month>
<year>2025</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2025 Remya, Suresh Kumar, Mithun, Praveen Kumar, Anoop, Reddem, Jeyakumar, Lotliker, Rao and Nair.</copyright-statement>
<copyright-year>2025</copyright-year>
<copyright-holder>Remya, Suresh Kumar, Mithun, Praveen Kumar, Anoop, Reddem, Jeyakumar, Lotliker, Rao and Nair</copyright-holder>
<license>
<ali:license_ref start_date="2025-10-30">https://creativecommons.org/licenses/by/4.0/</ali:license_ref>
<license-p>This is an open-access article distributed under the terms of the <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution License (CC BY)</ext-link>. The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</license-p>
</license>
</permissions>
<abstract>
<p>The Southern Ocean (SO) is a critical driver of global wave dynamics, generating long-period swells that propagate vast distances and significantly impact far distant coastal regions, including the Indian coastal regions. Climate change has intensified westerly winds and altered storm tracks in the Southern Hemisphere, resulting in higher wave heights and longer periods, which in turn increase the risk to coastal regions.&#x200b; However, the remote and harsh environment in the SO has historically limited <italic>in-situ</italic> wave observations, hindering a comprehensive understanding of the wave characteristics in the region. To bridge this gap, the Indian National Centre for Ocean Information Services (INCOIS) launched the Indian Ocean Wave Drifter (IOWD) program in 2021 under the Deep Ocean Mission to address the <italic>in-situ</italic> data gap in the Southern Indian Ocean. Through the deployment of GPS-enabled directional wave spectra drifters, the program has enabled near-real-time observations of wave characteristics across the SO. This article highlights the early outcomes of the IOWD program, including wave model validation, Stokes drift estimation, and swell tracking. The study emphasizes the importance of sustained <italic>in-situ</italic> observations from remote oceans for improving wave forecasting, enhancing coastal preparedness, and advancing scientific understanding of wave&#x2013;current interactions and climate variability in the Indian Ocean region.</p>
</abstract>
<kwd-group>
<kwd>directional wave spectra drifter</kwd>
<kwd>southern ocean</kwd>
<kwd>ocean surface waves</kwd>
<kwd>deep ocean mission</kwd>
<kwd>indian ocean wave drifter program</kwd>
</kwd-group>
<funding-group>
<funding-statement>The author(s) declare financial support was received for the research and/or publication of this article. The research and the IOWD program is funded by Ministry of Earth Science, Govt. of India.</funding-statement>
</funding-group>
<counts>
<fig-count count="10"/>
<table-count count="2"/>
<equation-count count="1"/>
<ref-count count="25"/>
<page-count count="13"/>
<word-count count="4986"/>
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<custom-meta-group>
<custom-meta>
<meta-name>section-in-acceptance</meta-name>
<meta-value>Ocean Observation</meta-value>
</custom-meta>
</custom-meta-group>
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</front>
<body>
<sec id="s1" sec-type="intro">
<label>1</label>
<title>Introduction</title>
<p>The Southern Ocean (SO) plays a pivotal role in global ocean dynamics and climate regulation due to its persistent strong winds, powerful currents, and extreme waves. Bounded by the Antarctic ice sheet to the south and major landmasses to the north, the SO features the planet&#x2019;s longest uninterrupted fetch, resulting in the generation of the largest and complex wave conditions anywhere on Earth. These waves, often exceeding 10 m in significant height, propagate across the ocean basins as long-period swells and act as global energy transporters (<xref ref-type="bibr" rid="B1">Babanin et&#xa0;al., 2019</xref>).</p>
<p>These swell systems have far-reaching impacts, far beyond their point of origin (<xref ref-type="bibr" rid="B19">Remya et&#xa0;al., 2016</xref>). The North Indian Ocean (NIO), particularly the southwest coast of India, is notably affected by SO-generated swells. Coastal flooding and freak wave incidents have been consistently linked with these remote swell events (<xref ref-type="bibr" rid="B18">Remya et&#xa0;al., 2012</xref>; <xref ref-type="bibr" rid="B13">Nayak et&#xa0;al., 2013</xref>; <xref ref-type="bibr" rid="B20">Sabique et&#xa0;al., 2012</xref>; <xref ref-type="bibr" rid="B17">Ramakrishnan et&#xa0;al., 2022</xref>). A growing body of literature demonstrated this relationship, including the arrival of Atlantic swells on the Indian coast (<xref ref-type="bibr" rid="B21">Samiksha et&#xa0;al., 2012</xref>) and the linkage between SO storms and Kallakadal-type flash flooding events along the Indian coast (<xref ref-type="bibr" rid="B19">Remya et&#xa0;al., 2016</xref>). Other studies (<xref ref-type="bibr" rid="B12">Majumder et&#xa0;al., 2022</xref>; <xref ref-type="bibr" rid="B16">Ramakrishnan et&#xa0;al., 2018</xref>) have highlighted the role of SO swells in coastal erosion and the formation of freak waves, which cause severe risks to marine operations and coastal infrastructure.</p>
<p>Climate change has further intensified the influence of SO on global wave patterns. Observations and model studies (<xref ref-type="bibr" rid="B22">Semedo et&#xa0;al., 2012</xref>; <xref ref-type="bibr" rid="B7">Hemer et&#xa0;al., 2013</xref>) have shown statistically significant increases in significant wave height and wave periods. The intensification and poleward migration of westerly wind belts and storm tracks drive these changes. This results in a global increase in the annual mean wave period, affecting over ~30% of the global Ocean and changes wave propagation directionality (<xref ref-type="bibr" rid="B7">Hemer et&#xa0;al., 2013</xref>). Another study by <xref ref-type="bibr" rid="B2">Bhaskaran et&#xa0;al. (2014)</xref> based on satellite measurements highlighted that the SO belt, between 40&#xb0;S &#x2013; 55&#xb0;S, experiences the highest variability due to climate change. These trends have profound implications for the Indian Ocean basin, exacerbating nonlinear interactions between wind sea and swell, increasing swell surges and freak waves, and amplifying the risks of extreme wave events.</p>
<p>Despite its global importance, SO remains the most under-observed region of the global Ocean. The extreme sea states, remote location and harsh environmental conditions (colloquially referred to as the &#x2018;Roaring Forties&#x2019; and &#x2018;Furious Fifties) pose significant challenges to sustained <italic>in situ</italic> observations. Satellite altimeters, although valuable, provide only limited data (mainly significant wave height) and lack the directional or spectral information necessary to understand the complexity of swell generation and propagation. Moored buoys are both logistically impractical and financially unsustainable in the harsh SO environments, which highlights the importance of wave drifters as a viable alternative for <italic>in-situ</italic> observations.</p>
<p>Wave drifters have already proven their utility in different ocean basins. <xref ref-type="bibr" rid="B24">Veras Guimar&#xe3;es et&#xa0;al. (2018)</xref> demonstrated that low-cost drifting buoys could capture wave&#x2013;current interactions in macro-tidal coastal environments. <xref ref-type="bibr" rid="B8">Hisaki (2021)</xref> validated drifting-buoy data against moored GPS buoys and ERA5 reanalysis near Japan, demonstrating that drifters provided more accurate wave heights in regions with strong currents. <xref ref-type="bibr" rid="B10">Houghton et&#xa0;al. (2021)</xref> further showed that a network of free-drifting Spotter buoys significantly enhanced wave forecast skill, reducing forecast errors and improving swell event detection. <xref ref-type="bibr" rid="B9">Holphe et&#xa0;al. (2025)</xref> compared wave displacements from a moored and a drifting Spotter buoy during an accidental voyage in the Indian Ocean, further demonstrating the robustness of drifting buoy measurements. More recently, <xref ref-type="bibr" rid="B25">Wu et&#xa0;al. (2025)</xref> used drifting buoys in the Kuroshio Extension to reveal how background currents modulate surface wave characteristics, while <xref ref-type="bibr" rid="B3">Cavaleri et&#xa0;al. (2025)</xref> highlighted the potential of small drifting buoys to resolve fine-scale processes such as wave steepness, breaking, and dissipation. Collectively, these studies demonstrate the versatility and reliability of drifting buoys for acquiring high-quality wave data in challenging ocean environments.</p>
<p>Building upon this global evidence, and to address the data scarcity in the Southern Indian Ocean (SIO), the Indian National Centre for Ocean Information Services (INCOIS), under the Ministry of Earth Sciences (MoES, Govt. of India), initiated the Indian Ocean Wave Drifter (IOWD) program in 2021 under its flagship Deep Ocean Mission (DOM). The primary objectives of the IOWD program are to (i) obtain <italic>in-situ</italic> wave spectra information from the SIO, (ii) reduce observational gaps that limit wave model accuracy in the IO, and (iii) provide datasets to improve both scientific understanding of wave climate variability and operational forecasting. The program employs GPS-based Directional Wave Spectra Drifters (DWSD), developed by the Lagrangian Drifter Laboratory (LDL) at Scripps Institution of Oceanography. The deployment of DWSDs represents a major step forward in addressing the observational gap in SIO and enhancing our understanding of wave dynamics. The IOWD program not only supports scientific advancement and operational forecasting, which are aimed at as the immediate priorities, but also contributes directly to several of the United Nations Sustainable Development Goals (SDGs). It addresses the SDG13 (Climate action) by providing critical data for monitoring and modelling climate induced changes in the ocean; SDG14 (life below water) by supporting ocean health and ecosystem resilience through better wave and current forecasting; and SDG 9 (industry innovation and infrastructure) through the deployment of cutting-edge observational technologies and infrastructure in extreme marine environments.</p>
<p>This article introduces the IOWD program, describes the technical specifications of the DWSDs, outlines the multi-phase implementation strategy, and presents key early applications. These include wave model validation, swell tracking, and Stokes drift estimation, all of which demonstrate the potential of sustained <italic>in-situ</italic> wave observation in the SO and Indian Ocean region.</p>
</sec>
<sec id="s2">
<label>2</label>
<title>DWSD technical overview</title>
<p>The Directional Wave Spectra Drifter (DWSD) is a compact, free-drifting, Lagrangian platform designed by the Lagrangian Drifter Laboratory (LDL) at the Scripps Institution of Oceanography (<xref ref-type="bibr" rid="B14">Postacchini et&#xa0;al., 2015</xref>; <xref ref-type="bibr" rid="B4">Centurioni, 2017</xref>; <xref ref-type="bibr" rid="B5">Centurioni et&#xa0;al., 2017</xref>). These compact, cost-effective drifters can transmit real-time, high resolution directional wave spectra and ancillary data from remote and other inaccessible ocean regions.</p>
<p>The DWSD, which weighs 12 kg, consists of a 0.39 m diameter spherical hull that houses a GPS receiver, batteries, data acquisition electronics, and an Iridium satellite modem (<xref ref-type="fig" rid="f1"><bold>Figure&#xa0;1</bold></xref>). It is powered by replaceable alkaline or lithium batteries, offering extended mission durations, depending on the sampling duration and environmental conditions. The GPS sensor in the DWSD records 3D velocity time series (zonal and meridional), at a sampling rate of 2 Hz for 17 minutes every hour. The power spectral density, co-spectra and quadrature-spectra parameters are derived with the Fourier transforms of the correlation functions of each pair of the velocity time-series, giving the first five independent Fourier coefficients (a0, a1, a2, b1, b2) and thus the wave spectra for each hourly sea state. The drifter transmits data in real-time via the Iridium satellite system, including Significant wave height (Hs), Mean wave period (Tm), Mean wave direction (Mdir), Peak wave period (Tp), Peak wave direction (Pdir) and wave spectra. Metadata, such as timestamp, location, battery voltage, sea level pressure, and sea surface temperature, is also included in the data stream. Using two-way communication via Iridium, the sampling strategy can be reconfigured, allowing adaptive observation strategies in response to evolving ocean conditions.</p>
<fig id="f1" position="float">
<label>Figure&#xa0;1</label>
<caption>
<p>Wave drifter schematic diagram (Image courtesy: Lagrangian Drifter Laboratory).</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g001.tif">
<alt-text content-type="machine-generated">Diagram of a DWSBD buoy showing labeled components. The topfeatures an ABS Barometric Pressure Port above an ABS Hemisphere. A Stainless SteelSealing Band divides the hemisphere from the lower half, which includes an Eyebolt forNearshore Mooring Applications and a Sea Surface Temperature Sensor at the bottom.</alt-text>
</graphic>
</fig>
<p>To ensure the accuracy and reliability of the drifter data, a comprehensive quality control procedure was implemented. Data from the initial test phase was excluded to remove potential anomalies and inconsistencies. Outliers were identified and eliminated based on a threshold of five times the standard deviation to preserve data integrity. Additionally, any data points with zero and stuck values were discarded. The geographic positions of the drifters were verified to ensure they fell within the designated oceanic domain. This multi-step quality control process ensured that only high-quality, consistent data were retained for subsequent analysis (<xref ref-type="fig" rid="f2"><bold>Figure&#xa0;2</bold></xref>).</p>
<fig id="f2" position="float">
<label>Figure&#xa0;2</label>
<caption>
<p><bold>(A)</bold> Flowchart of the quality control procedure applied to drifter data <bold>(B)</bold> Comparison of raw drifter data and quality-controlled data.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g002.tif">
<alt-text content-type="machine-generated">Flowchart and line chart are displayed. The flowchart in section (a)details data processing steps: starting with raw drifter data, excluding test phase data,spike detection and removal, excluding zero-value records, verifying geographicpositions, and resulting in final quality-controlled data. The line chart in section (b) showssignificant wave height over time, comparing data before quality control in blue and afterin dashed yellow.</alt-text>
</graphic>
</fig>
</sec>
<sec id="s3">
<label>3</label>
<title>Indian Ocean Wave Drifter program</title>
<p>The IOWD program was initiated in 2021 under DOM by MoES, Govt. of India, aimed at exploring and harnessing the vast potential of the depths of the Ocean through a mission-mode approach. It focuses on six key themes: development of technologies for deep-sea mining and underwater robotics, ocean climate change advisory services, sustainable use of marine bio-resources, deep ocean survey and exploration, extraction of energy and freshwater from the Ocean, and establishing an advanced marine station for ocean biology. INCOIS is leading the development of climate change advisory services, and the drifter program is a part of this vertical. The program was started under the DOM in 2021. IOWD is envisaged as a continuous program, with 30 drifter deployments planned every year. The implementation so far has been carried out in multiple phases, leveraging the cruise opportunities to optimize the spatial coverage and data return. The continuing IOWD program can fill the critical gap in obtaining observed wave spectra from the SO, providing essential insights into the changing wave dynamics and climate perspective of this remote and challenging region.</p>
<p>The initial phase involved the deployment of 4 DWSD during the Southern Ocean Expedition by the National Centre for Polar and Ocean Research (NCPOR) in 2021, onboard MV Vasily Golovnin, targeting the high swell regions of the Southern Indian Ocean (SIO). These deployments provided valuable insights into early mission planning, system endurance and real-time telemetry. Subsequent deployments occurred in 2023 and 2024, expanding the geographic scope and increasing the number of drifters. A fleet of 30 drifters was deployed from RV Roger Revelle (20 numbers) and ORV Sagar Nidhi (10 numbers), covering the SIO and tropical Indian Ocean basins, respectively. These deployments were carefully planned to enable long period swell tracking from the SIO into the tropical oceans.</p>
<p>In addition to targeting swell propagating tracks, the program also focuses on deployments in areas influenced by mesoscale eddies and strong boundary currents to examine the wave-current interactions. During the 2024&#x2013;2025 Antarctic expedition, 3 drifters were deployed in the marginal ice zones to study the wave-ice interactions.</p>
<p><xref ref-type="fig" rid="f3"><bold>Figure&#xa0;3</bold></xref> shows along-track Hs values of the drifters from first, second and third phase deployments. It is evident from the figures that the drifters are effectively covering the remote areas and transmitting the data for a long period. The longest continuous dataset lasted 292 days, with most drifters functioning for more than six months&#x2014;highlighting their significance in remote wave observations. Real-time data reception and remote configurability allowed the research team to optimize sampling schedules and adapt to evolving weather and wave conditions. The cumulative data return has established a high resolution, multi-season observational archive that supports not only basic research and validation, but also operational oceanography.</p>
<fig id="f3" position="float">
<label>Figure&#xa0;3</label>
<caption>
<p>Wave drifter tracks of first, second and third phase deployment in the Indian Ocean; color represents significant wave height (m) along the tracks.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g003.tif">
<alt-text content-type="machine-generated">Map of the Indian Ocean displaying wave drifter tracks in the IOWD program; color represents significant wave height (m). Blue indicates lower intensity, while red shows higher intensity, with the scale ranging from zero to five point five on the right.</alt-text>
</graphic>
</fig>
</sec>
<sec id="s4">
<label>4</label>
<title>A few key applications of the IOWD program</title>
<p>In the following section, we highlight a few key applications of the IOWD program, using the DWSD data from the first phase deployment. These examples demonstrate the value of the program and its impact on advancing wave research. Although all drifters were initially deployed in the SIO, one drifter (drifter 4) drifted into the Atlantic Ocean, while the remaining three continued to operate within the SIO. The drifter tracks are shown in <xref ref-type="fig" rid="f4"><bold>Figure&#xa0;4A</bold></xref>. <xref ref-type="fig" rid="f4"><bold>Figure&#xa0;4B</bold></xref> presents the along-track time evolution of energy density recorded by the drifters. Notably, drifter 3 has provided a long data series spanning around 6 months until July 2021.</p>
<fig id="f4" position="float">
<label>Figure&#xa0;4</label>
<caption>
<p><bold>(A)</bold> Wave drifter tracks of initial deployment in the SO <bold>(B)</bold> Wave energy density along the drifter tracks.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g004.tif">
<alt-text content-type="machine-generated">Map and graphs showing wave drifter data. (a) Map with tracked paths of four drifters in the Indian Ocean, marked in pink, red, blue, and black. (b) Fourspectrograms displaying Wave energy density along the drifter tracks over time, labeled Drifter-1 to Drifter-4, with varying intensity color scales. Dates range from February 25 to July 25, 2021.</alt-text>
</graphic>
</fig>
<sec id="s4_1">
<label>4.1</label>
<title>Wave model validation</title>
<p>INCOIS runs a suite of wave models for various applications, including wave forecasting, climate service development, and wave research in the IO. The WAVEWATCH III model has been used for both global and regional wave forecasting applications. Until the initiation of the IOWD program, model studies relied on satellite altimeter-derived significant wave height (<inline-formula>
<mml:math display="inline" id="im1"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) for the validation of SO waves. Since the initiation of the drifter program, model results have now been validated using drifter wave parameters. <xref ref-type="fig" rid="f5"><bold>Figure&#xa0;5</bold></xref> shows the time series comparison of modeled wave parameters with drifter observations for a representative drifter, demonstrating good agreement across all parameters. Tm exhibits a slight negative bias, whereas Hs shows good agreement, even at the highest wave heights (&gt;10 m), proving the reliability of the model predictions in the southernmost latitudes. The observed mean wave direction (<inline-formula>
<mml:math display="inline" id="im2"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) was mostly within the range of 225&#xb0; &#x2013; 315&#xb0;, and the model-predicted values followed the same pattern. <xref ref-type="table" rid="T1"><bold>Table&#xa0;1</bold></xref> presents the model error statistics for the comparison, illustrating the good agreement between the model and drifter observations in the southern latitudes. From <xref ref-type="table" rid="T1"><bold>Table&#xa0;1</bold></xref>, it can be seen that the scatter index values are less than 0.25 for <inline-formula>
<mml:math display="inline" id="im3"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula>
<mml:math display="inline" id="im4"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula>
<mml:math display="inline" id="im5"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for all drifters, while <inline-formula>
<mml:math display="inline" id="im6"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> shows higher errors compared to the other parameters.</p>
<fig id="f5" position="float">
<label>Figure&#xa0;5</label>
<caption>
<p><bold>(A, B)</bold> Time series comparison of <inline-formula>
<mml:math display="inline" id="im7"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula>
<mml:math display="inline" id="im8"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of model and drifter observations along the track of Drifter 2 <bold>(C)</bold> wave rose plot for <inline-formula>
<mml:math display="inline" id="im9"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g005.tif">
<alt-text content-type="machine-generated">Two line graphs and two polar plots compare wave data. The topgraph (a) shows significant wave height from February to July with Drifter 2 and WW3 inred and blue. The bottom graph (b) shows mean wave period over the same time spansimilarly color-coded. The polar plots (c) display wave direction distribution for Drifter 2and WW3, with angles labeled from 0 to 360 degrees.</alt-text>
</graphic>
</fig>
<table-wrap id="T1" position="float">
<label>Table&#xa0;1</label>
<caption>
<p>Model error statistics for the drifter wave data comparison.</p>
</caption>
<table frame="hsides">
<thead>
<tr>
<th valign="middle" align="center">Name</th>
<th valign="middle" align="left">Parameters</th>
<th valign="middle" align="left">Mean bias</th>
<th valign="middle" align="left">Root mean square error</th>
<th valign="middle" align="left">Correlation coefficient</th>
<th valign="middle" align="left">Scatter index</th>
</tr>
</thead>
<tbody>
<tr>
<td valign="middle" rowspan="4" align="center">Drifter 1</td>
<td align="left"><inline-formula>
<mml:math display="inline" id="im10"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (m)</td>
<td align="right">0.19</td>
<td align="right">0.47</td>
<td align="right">0.89</td>
<td align="right">0.15</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im11"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (s)</td>
<td align="right">1.10</td>
<td align="right">2.31</td>
<td align="right">0.49</td>
<td align="right">0.21</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im12"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (s)</td>
<td align="right">-0.64</td>
<td align="right">0.90</td>
<td align="right">0.82</td>
<td align="right">0.11</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im13"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (deg)</td>
<td align="right">-5.93</td>
<td align="right">35.65</td>
<td align="right">0.73</td>
<td align="right">0.64</td>
</tr>
<tr>
<td valign="middle" rowspan="4" align="center">Drifter 2</td>
<td align="left"><inline-formula>
<mml:math display="inline" id="im14"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (m)</td>
<td align="right">0.40</td>
<td align="right">0.65</td>
<td align="right">0.93</td>
<td align="right">0.16</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im15"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (s)</td>
<td align="right">0.78</td>
<td align="right">1.92</td>
<td align="right">0.58</td>
<td align="right">0.17</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im16"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (s)</td>
<td align="right">-0.64</td>
<td align="right">0.79</td>
<td align="right">0.88</td>
<td align="right">0.09</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im17"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (deg)</td>
<td align="right">0.09</td>
<td align="right">20.96</td>
<td align="right">0.77</td>
<td align="right">0.70</td>
</tr>
<tr>
<td valign="middle" rowspan="4" align="center">Drifter 3</td>
<td align="left"><inline-formula>
<mml:math display="inline" id="im18"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (m)</td>
<td align="right">0.47</td>
<td align="right">0.72</td>
<td align="right">0.92</td>
<td align="right">0.19</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im19"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (s)</td>
<td align="right">1.19</td>
<td align="right">2.31</td>
<td align="right">0.47</td>
<td align="right">0.20</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im20"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (s)</td>
<td align="right">-0.59</td>
<td align="right">0.79</td>
<td align="right">0.86</td>
<td align="right">0.09</td>
</tr>
<tr>
<td align="left"><inline-formula>
<mml:math display="inline" id="im21"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (deg)</td>
<td align="right">1.42</td>
<td align="right">27.73</td>
<td align="right">0.74</td>
<td align="right">0.72</td>
</tr>
</tbody>
</table>
</table-wrap>
<p>At times, the drifter was located within storm-affected regions, where it measured high-energy spectra that were subsequently used for model validation. <xref ref-type="fig" rid="f6"><bold>Figure&#xa0;6</bold></xref> shows two such examples involving Drifter 2 and Drifter 3. In the first case, Drifter 2 was in a region of strong storm-induced winds and recorded a peak energy density of approximately 320 m&#xb2;/Hz. Although the model captured the overall spectral shape, it was unable to reproduce the peak of spectral energy density observed at 03 UTC on 14 June. However, the model did simulate peak spectral energy density of ~160 m&#xb2;/Hz at 12 UTC on the same day.</p>
<fig id="f6" position="float">
<label>Figure&#xa0;6</label>
<caption>
<p>(Left panel) One dimensional wave spectra comparison of model and wave drifter during two storm cases on 14<sup>th</sup> June (drifter 2) and 28<sup>th</sup> July (drifter 3), 2021; (Right panel) wind speed and direction in the storm area and the black spot shows drifter positions.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g006.tif">
<alt-text content-type="machine-generated">Four panel image featuring spectral energy density graphs on the left and corresponding wind maps on the right. The graphs show red and blue linesrepresenting Drifter 2 or 3 and WW3 data against frequency in Hertz, and spectral energydensity in meters squared per Hertz. Wind maps display colored contours indicating windspeed from 1.0 to 28.0 meters per second with vectors showing direction, ranging from30 to 60 degrees south and 30 to 120 degrees east. Dates for each panel are June 14,2021, at 03:00 and 12:00 UTC, and July 28, 2021, at 06:00 and 21:00 UTC.</alt-text>
</graphic>
</fig>
<p>In the second case, Drifter 3 was in a storm region on 28 July 2021. Like the first case, the model failed to reproduce the observed peak spectral energy density (~170 m&#xb2;/Hz) at 06 UTC, although it closely matched the observed spectra at 21 UTC on the same day. The errors in simulating storm-induced wave fields are largely attributed to inaccuracies in forecast wind inputs, as well as inadequacies in the parameterization schemes used in the model (<xref ref-type="bibr" rid="B15">Raj et&#xa0;al., 2023</xref>).</p>
<p>A potential solution to address these uncertainties is the assimilation of observational data. As seen in <xref ref-type="fig" rid="f6"><bold>Figure&#xa0;6</bold></xref>, the drifters effectively captured the highest energy levels during storm conditions, and assimilating such data can substantially improve wave forecasts. Increasing the number of drifter deployments in the SIO will enhance opportunities to capture such events and contribute to more accurate forecasting of wave fields and swell propagation in the region.</p>
</sec>
<sec id="s4_2">
<label>4.2</label>
<title>Tracking of the SO swells</title>
<p>One of the main objectives of the drifter program was the utilization of data for tracking and the study of the SO swells. The SO swells are controlling the NIO wave characteristics and have a significant impact on the Indian coastal areas. The changing patterns of swells due to climate change can have a significant impact on Indian coastal regions in terms of flooding and coastal erosion. Since there are no swell fields available from satellite altimeters/synthetic aperture radar directly, SO swell validation is unattainable. We have used a constant threshold frequency criterion (0.1 Hz) and made the sea and swell separation both from model and drifter. The validation of separated wave fields is shown in <xref ref-type="fig" rid="f7"><bold>Figure&#xa0;7</bold></xref>. As seen in <xref ref-type="fig" rid="f3"><bold>Figure&#xa0;3</bold></xref>, Drifter 2 tracks fall within a high wave height and swell-dominated regime and are therefore chosen as a representative track for the validation. The swell wave fields show close agreement with the drifter data, even during periods of high swell wave heights, whereas the swell wave period is overestimated, indicating an energy shift towards the lower-frequency part of the spectrum in the wave model (<xref ref-type="fig" rid="f7"><bold>Figure&#xa0;7</bold></xref>). Wind sea heights and periods were in good agreement with the observations. <xref ref-type="table" rid="T2"><bold>Table&#xa0;2</bold></xref> provides the error statistics of the model for the three drifters. The scatter index of the heights and periods of wind sea and swell is well below 0.3, indicating better performance of the forecast model in the SIO. Ocean current data were not included in the present wave model simulations, and this omission may have introduced biases, particularly in the South Indian Ocean, where strong currents are common. Future work will address wave&#x2013;current interactions in the Indian Ocean using drifter observations.</p>
<fig id="f7" position="float">
<label>Figure&#xa0;7</label>
<caption>
<p>Time series comparison of <inline-formula>
<mml:math display="inline" id="im22"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula>
<mml:math display="inline" id="im23"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of swell and wind sea of model and drifter observations along the track of drifter 2.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g007.tif">
<alt-text content-type="machine-generated">Four line graphs comparing wave and swell data from April 28 to July 20. The graphs show Swell \(Hs\) in meters, Wind Wave \(Hs\) in meters, Swell\(Tm\) in seconds, and Wind Wave \(Tm\) in seconds. Data is represented with red forDrifter 2 and blue for WW3.</alt-text>
</graphic>
</fig>
<table-wrap id="T2" position="float">
<label>Table&#xa0;2</label>
<caption>
<p>Model error statistics for the drifter wave data comparison.</p>
</caption>
<table frame="hsides">
<thead>
<tr>
<th valign="middle" align="center">Name</th>
<th valign="middle" align="left">Parameters</th>
<th valign="middle" align="left">Mean bias</th>
<th valign="middle" align="left">RMSE</th>
<th valign="middle" align="left">R</th>
<th valign="middle" align="left">Scatter index</th>
</tr>
</thead>
<tbody>
<tr>
<td valign="middle" rowspan="4" align="center">Drifter 1</td>
<td valign="middle" align="left">Swell <inline-formula>
<mml:math display="inline" id="im24"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.21</td>
<td valign="middle" align="right">0.65</td>
<td valign="middle" align="right">0.77</td>
<td valign="middle" align="right">0.28</td>
</tr>
<tr>
<td valign="middle" align="left">Wind wave <inline-formula>
<mml:math display="inline" id="im25"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">-0.03</td>
<td valign="middle" align="right">0.35</td>
<td valign="middle" align="right">0.88</td>
<td valign="middle" align="right">0.13</td>
</tr>
<tr>
<td valign="middle" align="left">Swell <inline-formula>
<mml:math display="inline" id="im26"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.90</td>
<td valign="middle" align="right">1.05</td>
<td valign="middle" align="right">0.71</td>
<td valign="middle" align="right">0.09</td>
</tr>
<tr>
<td valign="middle" align="left">Wind wave <inline-formula>
<mml:math display="inline" id="im27"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">-0.09</td>
<td valign="middle" align="right">0.31</td>
<td valign="middle" align="right">0.74</td>
<td valign="middle" align="right">0.05</td>
</tr>
<tr>
<td valign="middle" rowspan="4" align="center">Drifter 2</td>
<td valign="middle" align="left">Swell <inline-formula>
<mml:math display="inline" id="im28"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.37</td>
<td valign="middle" align="right">0.71</td>
<td valign="middle" align="right">0.91</td>
<td valign="middle" align="right">0.23</td>
</tr>
<tr>
<td valign="middle" align="left">Wind wave <inline-formula>
<mml:math display="inline" id="im29"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.14</td>
<td valign="middle" align="right">0.36</td>
<td valign="middle" align="right">0.90</td>
<td valign="middle" align="right">0.11</td>
</tr>
<tr>
<td valign="middle" align="left">Swell <inline-formula>
<mml:math display="inline" id="im30"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.83</td>
<td valign="middle" align="right">0.97</td>
<td valign="middle" align="right">0.73</td>
<td valign="middle" align="right">0.08</td>
</tr>
<tr>
<td valign="middle" align="left">Wind wave <inline-formula>
<mml:math display="inline" id="im31"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.01</td>
<td valign="middle" align="right">0.27</td>
<td valign="middle" align="right">0.72</td>
<td valign="middle" align="right">0.04</td>
</tr>
<tr>
<td valign="middle" rowspan="4" align="center">Drifter 3</td>
<td valign="middle" align="left">Swell <inline-formula>
<mml:math display="inline" id="im32"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.46</td>
<td valign="middle" align="right">0.74</td>
<td valign="middle" align="right">0.89</td>
<td valign="middle" align="right">0.29</td>
</tr>
<tr>
<td valign="middle" align="left">Wind wave <inline-formula>
<mml:math display="inline" id="im33"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.15</td>
<td valign="middle" align="right">0.37</td>
<td valign="middle" align="right">0.89</td>
<td valign="middle" align="right">0.13</td>
</tr>
<tr>
<td valign="middle" align="left">Swell <inline-formula>
<mml:math display="inline" id="im34"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">0.92</td>
<td valign="middle" align="right">1.09</td>
<td valign="middle" align="right">0.61</td>
<td valign="middle" align="right">0.09</td>
</tr>
<tr>
<td valign="middle" align="left">Wind wave <inline-formula>
<mml:math display="inline" id="im35"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></td>
<td valign="middle" align="right">-0.02</td>
<td valign="middle" align="right">0.29</td>
<td valign="middle" align="right">0.74</td>
<td valign="middle" align="right">0.04</td>
</tr>
</tbody>
</table>
</table-wrap>
</sec>
<sec id="s4_3">
<label>4.3</label>
<title>DWSD derived stokes drift and model comparison</title>
<p>During its periodic motion, a particle floating at the free surface of a water wave experiences a net drift velocity in the direction of wave propagation, known as the Stokes drift (<xref ref-type="bibr" rid="B23">Stokes, 1847</xref>). Ocean surface waves mainly contribute to turbulent kinetic energy and turbulent mixing throughout the mixed layer through Stokes drift and wave breaking. The Stokes drift is considered as an important parameter in the ocean-wave coupled model for representing the Langmuir effect. Additionally, Stokes drift is considered as an important parameter in the particle tracking model. It also plays a significant role in wave-induced turbulent mixing within climate system models (<xref ref-type="bibr" rid="B6">Fan et&#xa0;al., 2023</xref>). In the first few meters below the surface, Stokes drift influences the motion of drifters with shallow drogue and drifter observations allow the calculation of Stokes drift and the methodology is as follows.</p>
<p>If the one-dimensional variance spectra is used, the Stokes drift can be computed as (<xref ref-type="bibr" rid="B11">Kenyon, 1969</xref>):</p>
<disp-formula id="eq1"><label>(1)</label>
<mml:math display="block" id="M1"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>u</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>&#x2192;</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mn>16</mml:mn><mml:msup><mml:mi>&#x3c0;</mml:mi><mml:mn>3</mml:mn></mml:msup></mml:mrow><mml:mi>g</mml:mi></mml:mfrac><mml:mo>&#x222c;</mml:mo><mml:msup><mml:mi>f</mml:mi><mml:mn>3</mml:mn></mml:msup><mml:msub><mml:mi>E</mml:mi><mml:mrow><mml:mi>v</mml:mi><mml:mi>a</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>f</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>&#xa0;</mml:mo><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mfrac><mml:mrow><mml:mn>8</mml:mn><mml:msup><mml:mi>&#x3c0;</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:msup><mml:mi>f</mml:mi><mml:mn>2</mml:mn></mml:msup></mml:mrow><mml:mi>g</mml:mi></mml:mfrac><mml:mi>z</mml:mi></mml:mrow></mml:msup><mml:mi>d</mml:mi><mml:mi>f</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math>
</disp-formula>
<p>where <italic>g</italic> is gravity and <italic>z</italic> is the water depth, negative downward, f is the frequency, <italic>E<sub>var</sub></italic>, one dimensional wave spectrum.</p>
<p>Using <xref ref-type="disp-formula" rid="eq1">Equation 1</xref>, Stokes drift has been computed from the drifter data for three drifters and is shown in <xref ref-type="fig" rid="f8"><bold>Figure&#xa0;8</bold></xref>. The analysis shows maximum Stokes drift values near the surface, decreasing with depth, consistent with theoretical expectations. The WW3 model also provides surface Stokes drift. Therefore, the computed surface Stokes drift from the drifters is used to validate the WW3 model-derived Stokes drift (<xref ref-type="fig" rid="f9"><bold>Figure&#xa0;9</bold></xref>). The model shows good agreement with the drifter data, with a slight negative bias along all three drifter tracks, demonstrating the reliability of the model-derived surface Stokes drift. This validation builds confidence in using the model data for coupling applications and as input for particle tracking models.</p>
<fig id="f8" position="float">
<label>Figure&#xa0;8</label>
<caption>
<p>Stokes drift magnitude computed from drifter one dimensional wave spectrum.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g008.tif">
<alt-text content-type="machine-generated">Three heatmaps labeled Drifter-1, Drifter-2, and Drifter-3 display depth data in meters  and stokes drift along the depth from February 26, 2021, to July 26, 2021. Color indicate stokes drift values, with blue representing lower values and red indicating higher. The color scale ranges from 0.00 to 0.45 on the right.</alt-text>
</graphic>
</fig>
<fig id="f9" position="float">
<label>Figure&#xa0;9</label>
<caption>
<p>Comparison of model derived stokes drift (m/s) with wave drifter derived stokes drift (m/s).</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g009.tif">
<alt-text content-type="machine-generated">Line graphs compare observed and modeled stokes drift for three drifters from April 2 to April 30,2021. Each graph shows red lines for observed data and bluelines for modeled data.</alt-text>
</graphic>
</fig>
</sec>
</sec>
<sec id="s5">
<label>5</label>
<title>Real-time applications and future research directions</title>
<p>The Indian Ocean Wave Drifter (IOWD) program has already demonstrated substantial potential for integration into real-time operational forecasting systems and long-term climate monitoring. One of the immediate applications of the DWSD has been the real-time validation of daily forecasts. <xref ref-type="fig" rid="f10"><bold>Figure&#xa0;10</bold></xref> illustrates one example of real-time validation of the INCOIS wave forecast using drifter data from a remote location, as displayed on the website <uri xlink:href="https://www.incois.gov.in">www.incois.gov.in</uri>. The availability of near-real-time wave data has enabled operational forecast centers to assess model performance under varying sea conditions. This validation enables the credibility of wave forecast products disseminated to end users. Another near-future operational application is the assimilation of DWSD data in operational models.</p>
<fig id="f10" position="float">
<label>Figure&#xa0;10</label>
<caption>
<p>Real time validation of wave forecast (<inline-formula>
<mml:math display="inline" id="im36"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) with drifter data.</p>
</caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fmars-12-1642772-g010.tif">
<alt-text content-type="machine-generated">Line graph showing significant wave height in meters over timefrom May 2 to May 18, 2025. Red line represents drifter data, and blue line represents modeldata. Both lines start around 1.5 meters, dip slightly, and gradually increase, peaking at 3.5meters around May 16.</alt-text>
</graphic>
</fig>
<p>The IOWD dataset also supports the development of improved warning systems for swell-induced coastal hazards. By capturing the spectral and directional characteristics of incoming swell waves, the drifters provide key inputs for inferring regional-scale wave forecasts. This contributes to early warnings for Kallakkadal-type events and other forms of coastal flooding. The real-time transmission of data from remote ocean regions fills a critical observation gap that previously limited the accuracy of such warnings.</p>
<p>Looking ahead, the IOWD data archive is expected to serve as a reference dataset for evaluating long-term trends in wave energy and spectral characteristics. This is particularly relevant for understanding the influence of climate change on the SO wave climate and its teleconnections to the Indian Ocean. Future deployments will include targeted campaigns in polar and tropical zones, enabling studies of wave-ice interactions, mixed wave-current regimes, and air-sea exchange processes. Furthermore, there is significant scope for coupling DWSD observations with other oceanographic datasets, such as those from Argo floats, gliders, satellite altimetry, eddy covariance sensors etc. This multi-platform synergy will enable comprehensive assessments of wave-current interactions, upper ocean mixing, and momentum transfer. The drifters also hold promises to improve Stokes drift estimates, which are essential for applications ranging from marine pollution tracking to search-and-rescue operations.</p>
</sec>
<sec id="s6">
<label>6</label>
<title>Summary and way forward</title>
<p>The Indian Ocean Wave Drifter (IOWD) program is an important initiative for addressing a long-standing gap in <italic>in-situ</italic> observations across the Indian ocean, particularly in areas where <italic>in-situ</italic> mooring deployments are not feasible. The Southern Ocean (SO), a region critical to global wave generation and climate regulation, remains especially under sampled due to its remoteness and harsh conditions. The IOWD program, launched in 2021, under the Deep Ocean Mission (DOM) of MoES, aims to overcome these challenges by deploying GPS-based Directional Wave Spectra Drifters (DWSD), capable of transmitting wave spectra, sea level pressure and sea surface temperature from remote areas, in near-real time.</p>
<p>The program has already enabled several high-impact applications including validation of wave forecast models, data assimilation, tracking of long-period swells, estimation of Stokes drift, etc. The availability of wave spectra observations from remote and data-scarce regions will significantly advance our understanding of swell propagation in the IO, its role in coastal flooding, and the dynamics of wave&#x2013;current interaction.</p>
<p>Despite its successes, the IOWD program also faces several operational challenges. A notable percentage of deployed drifters have been affected with vandalism, beaching, and premature death limiting their effective life span and data continuity. Even though 37% of the 64 DWSD worked more than 250 days. Retrieval and redeployment operations are resource intensive and logistically demanding. Additionally, consistent access to ideal deployment tracks in the SO regions remains a major constraint, often hindering the deployment of drifters in key swell-generating zones. These challenges underscore the need for robust deployment planning and international collaboration, including coordinated ship time and shared observation strategies.</p>
<p>The broader implications of the IOWD program are substantial. By improving wave forecast accuracy in one of the most dynamic wave-generating regions, the program directly contributes to marine safety, the protection of coastal infrastructure, and enhanced disaster preparedness. Accurate wave predictions support early warnings for swell surges and extreme wave events, reducing risks to maritime operations and vulnerable coastal communities. The real-time and long-term drifter observations also provide crucial inputs for global climate models, helping refine projections of sea level rise and wave climate under changing atmospheric conditions. In this way, the IOWD program supports more informed and actionable climate adaptation policies.</p>
<p>From a strategic perspective, the IOWD program reflects commitment of India to the United Nations Decade of Ocean Science and aligns with Sustainable Development Goals (SDG 9, 13 and 14). Through sustained operation and expansion, the program is expected to generate significant new research, particularly in wave dynamics of the Indian Ocean, and foster technological and scientific innovation in ocean observing systems. The program will continue under the framework of DOM, with plans to procure additional wave drifters yearly for deployment across various parts of the Indian Ocean&#x2014;particularly in key under-sampled regions. With continued support and collaboration, the IOWD program is poised to become a flagship contribution from India to the global ocean observing community, advancing wave forecasting, climate research and coastal resilience for years to come.</p>
</sec>
</body>
<back>
<sec id="s7" sec-type="data-availability">
<title>Data availability statement</title>
<p>The datasets presented in this study can be found in online repositories. The names of the repository/repositories and accession number(s) can be found below: Available through request <uri xlink:href="https://www.incois.gov.in/site/datainfo/OON.jsp">https://www.incois.gov.in/site/datainfo/OON.jsp</uri>.</p></sec>
<sec id="s8" sec-type="author-contributions">
<title>Author contributions</title>
<p>PGR: Visualization, Resources, Validation, Data curation, Project administration, Conceptualization, Formal Analysis, Writing &#x2013; review &amp; editing, Methodology, Investigation, Writing &#x2013; original draft, Software, Supervision. NK: Methodology, Writing &#x2013; review &amp; editing, Data curation, Resources, Project administration. SM: Formal Analysis, Visualization, Writing &#x2013; review &amp; editing, Validation. BK: Formal Analysis, Writing &#x2013; review &amp; editing, Writing &#x2013; original draft. TA: Formal Analysis, Visualization, Data curation, Writing &#x2013; review &amp; editing. VR: Data curation, Writing &#x2013; review &amp; editing. CJ: Data curation, Writing &#x2013; review &amp; editing. AL: Funding acquisition, Project administration, Writing &#x2013; review &amp; editing, Supervision. ER: Funding acquisition, Writing &#x2013; review &amp; editing, Project administration, Supervision. TM: Project administration, Writing &#x2013; review &amp; editing, Supervision, Funding acquisition.</p></sec>
<ack>
<title>Acknowledgments</title>
<p>We thank Dr. M Ravichandran, Secretary, MoES for his support. We acknowledge the support of Dr. Yogesh Ray, Scientist, NCPOR, Voyage leader and team for initial deployment. We thank Langragian drifter laboratory, Dr. Luca Centurioni and Dr. Lance Braasch for DWSD development and support. Thanks to Chief Scientist of R/V Roger Revelle (RR 2308), Voyage Leader of M/V Vasiliy Golovnin (44<sup>th</sup> ISEA), Chief Scientist of R/V Sindhu Sankalp for second and third phase deployments. This research and IOWD program falls under OCCAS-Deep Ocean Mission and is funded by Ministry of Earth Science, Govt. of India. We thank the developers of WAVEWATCH III NOAA/NCEP for providing the WAVEWATCH III source code (<ext-link ext-link-type="uri" xlink:href="https://polar.ncep.noaa.gov/waves/">https://polar.ncep.noaa.gov/waves/</ext-link>) and for their consistent efforts to improve the accuracy of this open-source spectral model. We used MIHIR HPC facility for the wave model experiments. We thank two reviewers for their critical comments and suggestions. This is INCOIS contribution number 591.</p>
</ack>
<sec id="s10" sec-type="COI-statement">
<title>Conflict of interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p></sec>
<sec id="s11" sec-type="ai-statement">
<title>Generative AI statement</title>
<p>The author(s) declare that no Generative AI was used in the creation of this manuscript.</p>
<p>Any alternative text (alt text) provided alongside figures in this article has been generated by Frontiers with the support of artificial intelligence and reasonable efforts have been made to ensure accuracy, including review by the authors wherever possible. If you identify any issues, please contact us.</p></sec>
<sec id="s12" sec-type="disclaimer">
<title>Publisher&#x2019;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p></sec>
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<p>Edited by: <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1695803">Jian Wang</ext-link>, Tianjin University, China</p></fn>
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