The European Space Agency’s Sentinel-1 synthetic aperture radar (SAR) image was acquired 13 h after the initial eruption. The SAR image (
Fig. 1b) shows IWs in the northern area of the volcano eruption location. SAR can observe IW because it modulates the surface gravity capillary waves and manifests as bright-dark bands on SAR images (
Alpers, 1985). The Sentinel-1 SAR data were provided by European Space Agency and are available at
https://scihub.copernicus.eu/dhus/#/home. Clear IW packets propagating in different directions are observed. The length of the IW crests ranges from less than 20 km to 67 km. The north propagating IWs are separated by Tofua Island, forming IW patterns similar to the IWs in the Dongsha Atoll of the South China Sea. The cross-interactions patterns imply that these IWs may not generate at a single source.
Figure 2 shows the synergy observation of IWs using the Moderate-resolution Imaging Spectroradiometer (MODIS) and Sentinel-1 images with a time difference of about 5 h. The propagation speed of IWs is about 0.95 m/s. We have taken the profiles along the black line on the Sentinel-1 SAR image, as shown in
Fig. 2. The characteristic wavelength of IWs ranges from 860.9 m to 1 530.4 m, which is the typical value of IWs. The length of the leading IW wave crest is 67 km.