Pengumuman: Semua project nonkomersial yang terdaftar untuk menggunakan Earth Engine sebelum
15 April 2025 harus
memverifikasi kelayakan nonkomersial untuk mempertahankan akses Earth Engine.
Algoritma Sentinel-1
Tetap teratur dengan koleksi
Simpan dan kategorikan konten berdasarkan preferensi Anda.
Sentinel-1 adalah
misi luar angkasa yang didanai oleh Uni Eropa dan dijalankan oleh European Space Agency
(ESA) dalam Program Copernicus. Sentinel-1 mengumpulkan citra radar (SAR) aperture sintetis
C-band dengan berbagai polarisasi dan resolusi. Karena data radar
memerlukan beberapa algoritma khusus untuk mendapatkan citra ortorektifikasi yang dikalibrasi,
dokumen ini menjelaskan pra-pemrosesan data Sentinel-1 di Earth Engine.
Data Sentinel-1 dikumpulkan dengan beberapa konfigurasi instrumen, resolusi, kombinasi band yang berbeda selama orbit naik dan turun. Karena
heterogenitas ini, biasanya perlu memfilter data ke
subset homogen sebelum memulai pemrosesan. Proses ini diuraikan di bawah pada bagian
Metadata dan Pemfilteran.
Untuk membuat subset data Sentinel-1 yang homogen, biasanya Anda perlu memfilter koleksi menggunakan properti metadata. Kolom metadata umum yang digunakan untuk
pemfilteran mencakup properti berikut:
transmitterReceiverPolarisation
: ['VV'], ['HH'], ['VV', 'VH'], atau
['HH', 'HV']
instrumentMode
: 'IW' (Interferometric Wide Swath), 'EW'
(Extra Wide Swath), atau 'SM' (Strip Map). Lihat
referensi
ini untuk mengetahui detailnya.
orbitProperties_pass
: 'ASCENDING' atau 'DESCENDING'
resolution_meters
: 10, 25, atau 40
resolution
: 'M' (sedang) atau 'H' (tinggi). Lihat
referensi
ini untuk mengetahui detailnya.
Kode berikut memfilter koleksi Sentinel-1 menurut properti transmitterReceiverPolarisation
, instrumentMode
, dan orbitProperties_pass
, lalu menghitung gabungan untuk beberapa kombinasi pengamatan yang ditampilkan di peta untuk menunjukkan pengaruh karakteristik ini terhadap data.
Editor Kode (JavaScript)
// Load the Sentinel-1 ImageCollection, filter to Jun-Sep 2020 observations.
var sentinel1 = ee.ImageCollection('COPERNICUS/S1_GRD')
.filterDate('2020-06-01', '2020-10-01');
// Filter the Sentinel-1 collection by metadata properties.
var vvVhIw = sentinel1
// Filter to get images with VV and VH dual polarization.
.filter(ee.Filter.listContains('transmitterReceiverPolarisation', 'VV'))
.filter(ee.Filter.listContains('transmitterReceiverPolarisation', 'VH'))
// Filter to get images collected in interferometric wide swath mode.
.filter(ee.Filter.eq('instrumentMode', 'IW'));
// Separate ascending and descending orbit images into distinct collections.
var vvVhIwAsc = vvVhIw.filter(
ee.Filter.eq('orbitProperties_pass', 'ASCENDING'));
var vvVhIwDesc = vvVhIw.filter(
ee.Filter.eq('orbitProperties_pass', 'DESCENDING'));
// Calculate temporal means for various observations to use for visualization.
// Mean VH ascending.
var vhIwAscMean = vvVhIwAsc.select('VH').mean();
// Mean VH descending.
var vhIwDescMean = vvVhIwDesc.select('VH').mean();
// Mean VV for combined ascending and descending image collections.
var vvIwAscDescMean = vvVhIwAsc.merge(vvVhIwDesc).select('VV').mean();
// Mean VH for combined ascending and descending image collections.
var vhIwAscDescMean = vvVhIwAsc.merge(vvVhIwDesc).select('VH').mean();
// Display the temporal means for various observations, compare them.
Map.addLayer(vvIwAscDescMean, {min: -12, max: -4}, 'vvIwAscDescMean');
Map.addLayer(vhIwAscDescMean, {min: -18, max: -10}, 'vhIwAscDescMean');
Map.addLayer(vhIwAscMean, {min: -18, max: -10}, 'vhIwAscMean');
Map.addLayer(vhIwDescMean, {min: -18, max: -10}, 'vhIwDescMean');
Map.setCenter(-73.8719, 4.512, 9); // Bogota, Colombia
Penyiapan Python
Lihat halaman
Lingkungan Python untuk mengetahui informasi tentang Python API dan penggunaan
geemap
untuk pengembangan interaktif.
import ee
import geemap.core as geemap
Colab (Python)
# Load the Sentinel-1 ImageCollection, filter to Jun-Sep 2020 observations.
sentinel_1 = ee.ImageCollection('COPERNICUS/S1_GRD').filterDate(
'2020-06-01', '2020-10-01'
)
# Filter the Sentinel-1 collection by metadata properties.
vv_vh_iw = (
sentinel_1.filter(
# Filter to get images with VV and VH dual polarization.
ee.Filter.listContains('transmitterReceiverPolarisation', 'VV')
)
.filter(ee.Filter.listContains('transmitterReceiverPolarisation', 'VH'))
.filter(
# Filter to get images collected in interferometric wide swath mode.
ee.Filter.eq('instrumentMode', 'IW')
)
)
# Separate ascending and descending orbit images into distinct collections.
vv_vh_iw_asc = vv_vh_iw.filter(
ee.Filter.eq('orbitProperties_pass', 'ASCENDING')
)
vv_vh_iw_desc = vv_vh_iw.filter(
ee.Filter.eq('orbitProperties_pass', 'DESCENDING')
)
# Calculate temporal means for various observations to use for visualization.
# Mean VH ascending.
vh_iw_asc_mean = vv_vh_iw_asc.select('VH').mean()
# Mean VH descending.
vh_iw_desc_mean = vv_vh_iw_desc.select('VH').mean()
# Mean VV for combined ascending and descending image collections.
vv_iw_asc_desc_mean = vv_vh_iw_asc.merge(vv_vh_iw_desc).select('VV').mean()
# Mean VH for combined ascending and descending image collections.
vh_iw_asc_desc_mean = vv_vh_iw_asc.merge(vv_vh_iw_desc).select('VH').mean()
# Display the temporal means for various observations, compare them.
m = geemap.Map()
m.add_layer(vv_iw_asc_desc_mean, {'min': -12, 'max': -4}, 'vv_iw_asc_desc_mean')
m.add_layer(
vh_iw_asc_desc_mean, {'min': -18, 'max': -10}, 'vh_iw_asc_desc_mean'
)
m.add_layer(vh_iw_asc_mean, {'min': -18, 'max': -10}, 'vh_iw_asc_mean')
m.add_layer(vh_iw_desc_mean, {'min': -18, 'max': -10}, 'vh_iw_desc_mean')
m.set_center(-73.8719, 4.512, 9) # Bogota, Colombia
m
Pra-pemrosesan Sentinel-1
Citra di 'COPERNICUS/S1_GRD'
Sentinel-1 Earth Engine
ImageCollection
terdiri dari scene Ground Range Detected
(GRD) Level-1 yang diproses menjadi koefisien backscatter (σ°) dalam
desibel (dB). Koefisien pantulan balik mewakili
area pantulan balik target (bagian radar) per unit area tanah. Karena dapat
bervariasi menurut beberapa urutan magnitudo, nilai ini dikonversi ke dB sebagai
10*log10σ°. Nilai ini mengukur apakah medan yang dipancarkan menyebarkan
radiasi gelombang mikro yang datang secara preferensial dari sensor SAR
dB < 0) atau ke arah sensor SAR dB > 0). Perilaku hamburan ini bergantung pada karakteristik fisik medan, terutama geometri elemen medan dan karakteristik elektromagnetiknya.
Earth Engine menggunakan langkah prapemrosesan berikut (seperti yang diterapkan oleh
Sentinel-1 Toolbox)
untuk mendapatkan koefisien backscatter di setiap piksel:
- Menerapkan file orbit
- Memperbarui metadata orbit dengan
file orbit
yang direstorasi (atau file orbit yang akurat jika file yang direstorasi tidak
tersedia).
- Penghapusan derau batas GRD
- Menghapus derau intensitas rendah dan data yang tidak valid di tepi scene.
(Per 12 Januari 2018)
- Penghapusan derau termal
- Menghapus derau tambahan di sub-swath untuk membantu mengurangi diskontinuitas
di antara sub-swath untuk scene dalam mode akuisisi multi-swath.
(Operasi ini tidak dapat diterapkan pada gambar yang dibuat sebelum Juli 2015)
- Penerapan nilai kalibrasi radiometrik
- Menghitung intensitas backscatter menggunakan parameter kalibrasi
sensor dalam metadata GRD.
- Koreksi medan (ortorektifikasi)
- Mengonversi data dari geometri rentang darat, yang tidak memperhitungkan medan, ke σ° menggunakan DEM SRTM 30 meter atau DEM ASTER untuk lintang tinggi (lebih besar dari 60° atau kurang dari -60°).
Catatan Set Data
- Penghalusan Terrain Radiometrik tidak diterapkan
karena artefak di lereng gunung.
- Koefisien backscatter tanpa satuan dikonversi ke dB
seperti yang dijelaskan di atas.
- Data SLC Sentinel-1 saat ini tidak dapat diserap, karena Earth Engine
tidak mendukung gambar dengan nilai kompleks karena ketidakmampuan
untuk menghitung rata-ratanya selama pembuatan piramida tanpa kehilangan informasi
fase.
- Aset GRD SM tidak diserap karena
fungsi
computeNoiseScalingFactor()
dalam
operasi penghapusan derau batas di toolbox S1 tidak mendukung mode SM.
Kecuali dinyatakan lain, konten di halaman ini dilisensikan berdasarkan Lisensi Creative Commons Attribution 4.0, sedangkan contoh kode dilisensikan berdasarkan Lisensi Apache 2.0. Untuk mengetahui informasi selengkapnya, lihat Kebijakan Situs Google Developers. Java adalah merek dagang terdaftar dari Oracle dan/atau afiliasinya.
Terakhir diperbarui pada 2025-07-25 UTC.
[null,null,["Terakhir diperbarui pada 2025-07-25 UTC."],[[["\u003cp\u003eSentinel-1, part of the Copernicus Programme, provides C-band SAR data for various applications.\u003c/p\u003e\n"],["\u003cp\u003ePre-processing of Sentinel-1 data in Earth Engine involves filtering by metadata and applying specific algorithms.\u003c/p\u003e\n"],["\u003cp\u003eMetadata filtering is crucial for creating a homogeneous subset of data based on polarization, instrument mode, and orbit properties.\u003c/p\u003e\n"],["\u003cp\u003eEarth Engine automatically applies preprocessing steps including orbit file application, noise removal, radiometric calibration, and terrain correction to Sentinel-1 GRD data.\u003c/p\u003e\n"],["\u003cp\u003eThe data represents backscatter coefficient (σ°) in decibels (dB) and undergoes several processing steps to derive this value.\u003c/p\u003e\n"]]],["Sentinel-1 data, collected by the European Space Agency, is pre-processed in Earth Engine to obtain calibrated imagery. Key actions include filtering the heterogeneous data using metadata properties like `transmitterReceiverPolarisation`, `instrumentMode`, `orbitProperties_pass`, `resolution_meters`, and `resolution`. This is demonstrated in code examples using JavaScript and Python, calculating temporal means for visualization. Preprocessing steps involve applying orbit files, removing noise, radiometric calibration, and terrain correction to derive the backscatter coefficient in decibels (dB).\n"],null,["# Sentinel-1 Algorithms\n\n[Sentinel-1](https://earth.esa.int/web/sentinel/missions/sentinel-1) is a\nspace mission funded by the European Union and carried out by the European Space Agency\n(ESA) within the Copernicus Programme. Sentinel-1 collects C-band synthetic aperture\nradar (SAR) imagery at a variety of polarizations and resolutions. Since radar data\nrequires several specialized algorithms to obtain calibrated, orthorectified imagery,\nthis document describes pre-processing of Sentinel-1 data in Earth Engine.\n\nSentinel-1 data is collected with several different instrument configurations,\nresolutions, band combinations during both ascending and descending orbits. Because\nof this heterogeneity, it's usually necessary to filter the data down to a\nhomogeneous subset before starting processing. This process is outlined below in the\n[Metadata and Filtering](/earth-engine/guides/sentinel1#metadata-and-filtering) section.\n\nMetadata and Filtering\n----------------------\n\nTo create a homogeneous subset of Sentinel-1 data, it will usually be necessary to\nfilter the collection using metadata properties. The common metadata fields used for\nfiltering include these properties:\n\n1. `transmitterReceiverPolarisation`: \\['VV'\\], \\['HH'\\], \\['VV', 'VH'\\], or \\['HH', 'HV'\\]\n2. `instrumentMode`: 'IW' (Interferometric Wide Swath), 'EW' (Extra Wide Swath) or 'SM' (Strip Map). See [this\n reference](https://sentinel.esa.int/web/sentinel/user-guides/sentinel-1-sar/acquisition-modes) for details.\n3. `orbitProperties_pass`: 'ASCENDING' or 'DESCENDING'\n4. `resolution_meters`: 10, 25 or 40\n5. `resolution`: 'M' (medium) or 'H' (high). See [this\n reference](https://sentinel.esa.int/web/sentinel/user-guides/sentinel-1-sar/resolutions/level-1-ground-range-detected) for details.\n\nThe following code filters the Sentinel-1 collection by\n`transmitterReceiverPolarisation`, `instrumentMode`, and\n`orbitProperties_pass` properties, then calculates composites for several\nobservation combinations that are displayed in the map to demonstrate how these\ncharacteristics affect the data.\n\n### Code Editor (JavaScript)\n\n```javascript\n// Load the Sentinel-1 ImageCollection, filter to Jun-Sep 2020 observations.\nvar sentinel1 = ee.ImageCollection('COPERNICUS/S1_GRD')\n .filterDate('2020-06-01', '2020-10-01');\n\n// Filter the Sentinel-1 collection by metadata properties.\nvar vvVhIw = sentinel1\n // Filter to get images with VV and VH dual polarization.\n .filter(ee.Filter.listContains('transmitterReceiverPolarisation', 'VV'))\n .filter(ee.Filter.listContains('transmitterReceiverPolarisation', 'VH'))\n // Filter to get images collected in interferometric wide swath mode.\n .filter(ee.Filter.eq('instrumentMode', 'IW'));\n\n// Separate ascending and descending orbit images into distinct collections.\nvar vvVhIwAsc = vvVhIw.filter(\n ee.Filter.eq('orbitProperties_pass', 'ASCENDING'));\nvar vvVhIwDesc = vvVhIw.filter(\n ee.Filter.eq('orbitProperties_pass', 'DESCENDING'));\n\n// Calculate temporal means for various observations to use for visualization.\n// Mean VH ascending.\nvar vhIwAscMean = vvVhIwAsc.select('VH').mean();\n// Mean VH descending.\nvar vhIwDescMean = vvVhIwDesc.select('VH').mean();\n// Mean VV for combined ascending and descending image collections.\nvar vvIwAscDescMean = vvVhIwAsc.merge(vvVhIwDesc).select('VV').mean();\n// Mean VH for combined ascending and descending image collections.\nvar vhIwAscDescMean = vvVhIwAsc.merge(vvVhIwDesc).select('VH').mean();\n\n// Display the temporal means for various observations, compare them.\nMap.addLayer(vvIwAscDescMean, {min: -12, max: -4}, 'vvIwAscDescMean');\nMap.addLayer(vhIwAscDescMean, {min: -18, max: -10}, 'vhIwAscDescMean');\nMap.addLayer(vhIwAscMean, {min: -18, max: -10}, 'vhIwAscMean');\nMap.addLayer(vhIwDescMean, {min: -18, max: -10}, 'vhIwDescMean');\nMap.setCenter(-73.8719, 4.512, 9); // Bogota, Colombia\n```\nPython setup\n\nSee the [Python Environment](/earth-engine/guides/python_install) page for information on the Python API and using\n`geemap` for interactive development. \n\n```python\nimport ee\nimport geemap.core as geemap\n```\n\n### Colab (Python)\n\n```python\n# Load the Sentinel-1 ImageCollection, filter to Jun-Sep 2020 observations.\nsentinel_1 = ee.ImageCollection('COPERNICUS/S1_GRD').filterDate(\n '2020-06-01', '2020-10-01'\n)\n\n# Filter the Sentinel-1 collection by metadata properties.\nvv_vh_iw = (\n sentinel_1.filter(\n # Filter to get images with VV and VH dual polarization.\n ee.Filter.listContains('transmitterReceiverPolarisation', 'VV')\n )\n .filter(ee.Filter.listContains('transmitterReceiverPolarisation', 'VH'))\n .filter(\n # Filter to get images collected in interferometric wide swath mode.\n ee.Filter.eq('instrumentMode', 'IW')\n )\n)\n\n# Separate ascending and descending orbit images into distinct collections.\nvv_vh_iw_asc = vv_vh_iw.filter(\n ee.Filter.eq('orbitProperties_pass', 'ASCENDING')\n)\nvv_vh_iw_desc = vv_vh_iw.filter(\n ee.Filter.eq('orbitProperties_pass', 'DESCENDING')\n)\n\n# Calculate temporal means for various observations to use for visualization.\n# Mean VH ascending.\nvh_iw_asc_mean = vv_vh_iw_asc.select('VH').mean()\n# Mean VH descending.\nvh_iw_desc_mean = vv_vh_iw_desc.select('VH').mean()\n# Mean VV for combined ascending and descending image collections.\nvv_iw_asc_desc_mean = vv_vh_iw_asc.merge(vv_vh_iw_desc).select('VV').mean()\n# Mean VH for combined ascending and descending image collections.\nvh_iw_asc_desc_mean = vv_vh_iw_asc.merge(vv_vh_iw_desc).select('VH').mean()\n\n# Display the temporal means for various observations, compare them.\nm = geemap.Map()\nm.add_layer(vv_iw_asc_desc_mean, {'min': -12, 'max': -4}, 'vv_iw_asc_desc_mean')\nm.add_layer(\n vh_iw_asc_desc_mean, {'min': -18, 'max': -10}, 'vh_iw_asc_desc_mean'\n)\nm.add_layer(vh_iw_asc_mean, {'min': -18, 'max': -10}, 'vh_iw_asc_mean')\nm.add_layer(vh_iw_desc_mean, {'min': -18, 'max': -10}, 'vh_iw_desc_mean')\nm.set_center(-73.8719, 4.512, 9) # Bogota, Colombia\nm\n```\n\nSentinel-1 Preprocessing\n------------------------\n\nImagery in the Earth Engine `'COPERNICUS/S1_GRD'` Sentinel-1\n`ImageCollection` is consists of Level-1 Ground Range Detected\n(GRD) scenes processed to backscatter coefficient (σ°) in\ndecibels (dB). The backscatter coefficient represents\ntarget backscattering area (radar cross-section) per unit ground area. Because it can\nvary by several orders of magnitude, it is converted to dB as\n10\\*log~10~σ°. It measures whether the radiated terrain scatters\nthe incident microwave radiation preferentially away from the SAR sensor\ndB \\\u003c 0) or towards the SAR sensor dB \\\u003e 0). This scattering behavior depends on the\nphysical characteristics of the terrain, primarily the geometry of the terrain elements\nand their electromagnetic characteristics.\n\nEarth Engine uses the following preprocessing steps (as implemented by the\n[Sentinel-1 Toolbox](https://sentinel.esa.int/web/sentinel/toolboxes/sentinel-1))\nto derive the backscatter coefficient in each pixel:\n\n1. **Apply orbit file**\n - Updates orbit metadata with a restituted [orbit file](https://sentinel.esa.int/web/sentinel/technical-guides/sentinel-1-sar/pod/products-requirements) (or a precise orbit file if the restituted one is not available).\n2. **GRD border noise removal**\n - Removes low intensity noise and invalid data on scene edges. (As of January 12, 2018)\n3. **Thermal noise removal**\n - Removes additive noise in sub-swaths to help reduce discontinuities between sub-swaths for scenes in multi-swath acquisition modes. (This operation cannot be applied to images produced before July 2015)\n4. **Application of radiometric calibration values**\n - Computes backscatter intensity using sensor calibration parameters in the GRD metadata.\n5. **Terrain correction** (orthorectification)\n - Converts data from ground range geometry, which does not take terrain into account, to σ° using the [SRTM 30 meter DEM](/earth-engine/datasets/catalog/USGS_SRTMGL1_003) or the [ASTER DEM](https://asterweb.jpl.nasa.gov/gdem.asp) for high latitudes (greater than 60° or less than -60°).\n\nDataset Notes\n-------------\n\n- Radiometric Terrain Flattening is not being applied due to artifacts on mountain slopes.\n- The unitless backscatter coefficient is converted to dB as described above.\n- Sentinel-1 SLC data cannot currently be ingested, as Earth Engine does not support images with complex values due to inability to average them during pyramiding without losing phase information.\n- GRD SM assets are not ingested because the `computeNoiseScalingFactor()` function in the [border noise removal operation in the S1 toolbox](https://github.com/senbox-org/s1tbx/blob/master/s1tbx-op-calibration/src/main/java/org/esa/s1tbx/calibration/gpf/RemoveGRDBorderNoiseOp.java) does not support the SM mode."]]