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Help / Frequently Asked Questions (FAQ)
How do I access the satellite data?What datasets are available?Information about Level 3 composites:MultiView website:Java Image Viewer:How do I extract data from images?Specific algorithms:Further information:
How do I access the satellite data?Registration only takes a few minutes and is possible here. After you have registered, you are given free access to certain images in our archive. Other products are restricted to certain groups of users. So if you see 'Restricted Access', it does not mean your password has stopped working; it just means that you are not authorised to view those particular products. Everyone can currently access these products:These products have restricted access:If, after reading the question below, you feel that you have been denied access to an image incorrectly, please contact us. There are several groups of users who have privileged access to some of the restricted products: If you are in the UK academic category, then you can apply for the data you need by filling in and posting to us a peer-review form (Word RTF format). If you are potentially in one of the other categories, please contact us for details, pricing quotations or to discuss research collaboration. If you have read the two questions above, but still think that your password is not working, please check your password before you contact us. Please do not fill out another registration form. NB If you do still need to contact us about an access problem, please include your username and the full URL (http://.../.../) of the page you were trying to access, otherwise it is difficult for us to help. Only SeaWiFS Authorised Research Users are permitted to access SeaWiFS ocean colour data. To become an authorised user you must apply to NASA, which takes about two weeks to be processed. After that please inform us by e-mail, then we will reply within two days to confirm that you have been initially granted access to view SeaWiFS quick-look images. For access to any additional products you must demonstrate that you are in one of the categories listed above. If you are not in any of these categories but require free data, you may order standard products directly from the NASA SeaWiFS web site. All data will be subject to a 14-day embargo, unless specifically approved by NASA for near-real time research usage. What datasets are available?
Table 1: Temporal availability for each sensor. Data from four different sensors are available through this site. The oldest of these is the AVHRR which was first launched in 1978 on-board the TIROS-N satellite. Subsequent launches of replacement satellites has allowed continual coverage from 1978 up to present day. Through this site we offer AVHRR sea surface temperature (SST) estimates at a spatial resolution of 4 km. The SeaWiFS sensor was launched in 1997 on-board the Orbview SeaStar satellite. SeaWiFS ocean colour products are available through this site including normalised water leaving radiance data (nLw), estimates of chlorophyll-a and K490 estimates all at a spatial resolution of 1 km. These data are no longer available to us in near-real time, however, an archive of data between 1997 and December 2004 is available. More recently NASA have launched two MODIS sensors known as MODIS Terra (launched in 1999) and MODIS Aqua (launched in 2002). On this website we refer to MODIS-Aqua data processed by NASA as 'MODIS-Aqua NASA', whereas 'MODIS-Aqua' refers to identical data that we have processed (these data are available up to 24 hours before the equivalent NASA data). The MODIS products include nLw, chlorophyll-a (for both case I and case II waters) and SST. Finally, we have recently obtained access to the MERIS data. This instrument was launched in 2002 onboard the European Space Agency's environmental monitoring satellite ENVISAT. These data are available at 1 km spatial resolution providing products including nLw and chlorophyll-a (for case 1 and case 2 waters).
You can find images in the Products Browser if you already know the contract name under which they are stored. For example, the 'pa' area covers Plymouth, and those data are produced for the 'PACE' contract; so choose one of the satellite sensors (e.g. 'modis'), then click on the 'pace' directory, then the year, month and day of the satellite pass you require. There is also a large area covering most of NW Europe which is only available as a composite SST image. There are many other areas which are not being routinely processed, but have been processed for certain periods in the past. Check the lower part of the area list and the browser, to see if your region and dates of interest have already been processed. Requests for other areas within the receiving range of Dundee Satellite Station can be processed at 1 km resolution. Any region outside this range can be processed at a reduced resolution (4 km for AVHRR). Please contact us for details. The <product> part of image filenames specifies what property is represented by the image values:
All images are navigated and warped to Mercator projection. Land, clouds, and sunglint are usually masked out in black, though users should be aware that clouds may occasionally escape detection, and appear as unnaturally cold sea regions. Sea-surface temperature (SST) images represent temperatures in the range 5.0 to 30.5 °C. In certain regions and conditions, the sea surface may become significantly warmer than the bulk SST during the day, so the earliest image in the morning usually gives the most reliable estimate. SST values can be derived from the image using the formula: SST = pixel value * 0.1 + 5.0 Weekly and monthly SST composite images are available for the following areas: Bay of Biscay, Iberian Peninsula, Celtic Sea, Irish Shelf, Galicia, and also a large area covering most of NW Europe. These are very useful for visualising dynamic structures and seasonal temperature distributions even in cloudy regions. A coloured version of each SST image ('...sstpcol.gif') is now produced automatically, so that most thermal structures can be seen immediately without additional enhancement. The colour palette is dynamically adjusted to visualise the temperature range on each image. This scheme is preferable to a fixed palette for images covering small geographic regions, as these usually have a small temperature range, though it does mean that colours may not be comparable between different images. We recommend the use of an image manipulation package for further contrast enhancement and magnification of regions of interest. We use XV for X Windows, and Paint Shop Pro for Windows. A textual information file ('..._xx%.txt') contains details of the time, size and coordinates of each image. The percentage of sea area which is cloud-free is appended to the filename, to assist the user in finding clear images. Clouds are masked from the images using the folllowing tests:
Water vapour products (in g cm-2) are calculated using the equation: w = 1.96 (T4 - T5) cos sva NEODAAS Level 1B to Level 2 conversionThe conversion is performed using a modified version of the SeaDAS module l2gen. A typical command line would have the form:
Processing methodology: Viewable Product FilesFor SeaWiFS the <product> part of image filename is split into several parts of the form <resolution>_<product>_F<col>. The resolution can be of the form:
The standard products are as follows, and are explained in more detail in NASA's MSL12 documentation.
We have an example data set to explain these products. All images are navigated and warped to Mercator projection. The <col> part shows whether the gif file has had a colour palette applied. It is important to note that colour palette (except for the nasa_chlor_a product) is dynamically adjusted to visualise the value range on each image. This means that colours may not be comparable between different images. SeaWiFS Algorithms used within SeaDASChlorophyll algorithm: OC4 version 4 (Maximum Band Ratio, 4th Order Polynomial) a = [0.366,-3.067,1.930,0.649,-1.532] R = ALOG10((Rrs443>Rrs490>Rrs510)/Rrs555) Chl a (ug/l) = 10.0^(a(0) + a(1)*R + a(2)*R^2 + a(3)*R^3 + a(4)*R^4) K_490 algorithm:
K_490 = k490_1 + k490_2 * ( nLw_443 / nLw_555 ) k490_3
Coefficients are: k490_1 0.022; k490_2 0.100; k490_3 -1.29966
HDF Product FilesThe mapped HDF files are generated using the SeaDAS module bl2map. The standard MODIS products are listed in this table, and are explained in more detail in NASA's MSL12 documentation.
Information about EO products:Part (or all) of the scene may contain no-data (appearing black) due to the existence of cloud and other aerosols between the sensor and the target (ocean or land). This will result in missing data as the majority of the data that we process are from visible spectrum sensors (400nm - 700nm). Data may be unavailable for the particular date and time (See "Why are there large areas of black (no-data) in these images?"). A further reason for lack of data is that the sensor did not pass over the region of interest. This occurs as the satellites have repeat cycles of 1-3 days (dependent on the satellite). This can mean that data are only available over a particular region (for a particular sensor) once every three days. MERIS data are most likely to be affected by this issue. Image filenames generated by Panorama are of the form <date><time><area><product>.gif, where the <product> types are described in the AVHRR and SeaWiFS sections below. Image filenames for these sensors are of the following form, and the product types are described in the MODIS and MERIS sections. MYYYYJJJ.HHMM.aa.product.sensor.DDmmmYYHHMM.version.YYYYJJJHHMM.palette.filetype where each filename component is explained as follows:
For AVHRR and SeaWiFS we use a system called Panorama, developed at RSG using C, UNIX and IDL. A description of Panorama was published in this paper. The system for MODIS and MERIS is described in this paper. The systems are not currently available for purchase. Panorama uses a sphere of diameter 6370718 meters to approximate the Earth's surface. This is used as the datum baseline for all mapped processing. The regional Molodensky offsets between the sphere and a WGS 84 ellipsoid based datum are available on request. Information about Level 3 composites:Navigate to the data you require using the the directory links at the top of the page. The composite products are organised in the following directory structure:
sensor/dataset/area-code/period/product/year where each directory component is explained as follows:
All level 3 composite files are named according to this format: MYYYYJJJ-YYYYJJJ.aa.product.sensor.composite-type.DDmmmYY-DDmmmYY.version.YYYYJJJTTTT.palette.filetype where each filename component is explained as follows:
MultiView website:
Table 2: Available products for each sensor.
Table 3: Available model products. Java Image Viewer:When you click on an image, the Java image viewer should load. If it does not, then you need to install a Java plugin for your browser (further information) When you select an image the Java image viewer will load showing a window onto your selected data. The scroll bars on the sides of the image will allow you to move around. Across the top of the viewer are a series of menus: file, view, zoom and overlay. The details of these are described below. FileSave as..: allows you save the current display as an image (supported formats include gif, png, bmp, jpeg, wbmp and ascii). If you did not accept the Java certificate the first time the image viewer loaded then this functionality will be disabled. Copy: allows you to copy the image to your clipbaord. If you did not accept the Java certificate the first time the image viewer loaded then this functionality will be disabled. ViewInteractive stretch: This tool is very simple yet remarkably powerful. It allows you to stretch and slide the colour palette which is helpful for viewing the fine detail in the images. The tool consists of a box with a diagonal line passing through it. This line represents the colour palette. When it passes through both the bottom-left and top-right corners of the box the palette is identical to the one stored in the image. If you drag the mouse around a bit and you will quickly get the idea. Right clicking will toggle the 'Interactive Stretch' tool on and off. Pixel values : This allows you to determine the parameters of the pixel directly underneath the mouse cursor. Parameters displayed are latitude, longitude, DN value, geophysical parameter (if appropriate) and its scale bar colour. Left clicking with the mouse on the image will cause the 'Pixel Values' tool window to toggle on and off. Colour table :This allows you to select and view a palette from a predefined selection. ZoomThis menu allows you zoom to one of five predefined levels, or to zoom to a custom level. Also the 'Fit' option will zoom the image to that it fits exactly within the available space. Alternatively you can zoom using the mouse wheel or by selecting a box around the desired area selectin the left mouse button and dragging. You can also zoom in and out using the mouse wheel if you have one, and you can zoom in to a specific area by dragging the left mouse button to draw the desired box. Overlay
This menu will vary depending on the image you are viewing, however the
'Grid' option is always available. The Grid option will overlay a labelled
lattitude/longitude grid onto the image. The labels of this grid will 'follow'
the currently viewed area. Some examples of the overlays are the Coastlines which draw the lines
where the land and sea meet.
You will need Sun's Java Runtime Environment which can be downloaded at the Sun Microsystems. You will need at least version 1.4.2 to be able to run the Image Viewer. The Image Viewer is a signed applet. This means that it has some features that are not normally available to applets and it needs your approval to enable these features. These features including 'Copy to clipboard' and Saving the image. Before the image viewer starts you may be asked if you trust the applet and wish to accept the certificate. If you choose 'Yes' or 'Always' these features will be enabled. If you answer 'No' then you will still be able to use the image viewer but these features will not work.
The following applet will give you information about your version of Java.
Microsoft ceased development on Microsoft Java and it is no longer supplied with Micorsoft Windows (WinXP/SP1
and later do not include Java). We recommend the use of Sun's Java using their JRE. The minimum version required for the Java image viewer on this site is v1.4.2.
This is an excellent JVM (it is Sun's JVM with some special Mac features added) however there are a
few non-technical issues to be aware of. The main one is that since Apple's JVM is so tightly
integrated into MacOS X, it is often the case that you need to upgrade OS X to be able to update
the JVM. Apple have recently released v5.0 of their JVM, however you need OS X 10.4 to be able to
install it. The minimum required JVM version is v1.4.2 which is packaged with OS X 10.3 and later. JVM
1.4.2 may be available on OS X 10.2 but I have been unable to confirm this (it is definitely not
available for 10.1 and earlier). Windows Users:You can download Sun's JVM 5.0 from here. It is up to you whether you choose the offline installation or the online version. For slow connections it is probably best to choose the offline installation so that you can back it up on to CD. Linux Users:You can download Sun's JVM 5.0 from here. If your distribution uses RedHat Package (i.e. you install things with an .rpm file) then select the 'RPM in self extracting file'. Otherwise select the normal 'self extracting file'. Mac OS X Users:You can download Apple's JVM 5.0 from here, you will need Mac OS X 10.4 to use it. Users of Mac OS X 10.3 (possibly 10.2 but we're not sure) can use Mac OS X instead. Before loading the image viewer you should install the JAI-ImageIO optional package. This is not a requirement however you will gain access to more image formats if it installed, most notably the TIFF format (which we plan to extend into GeoTIFF in the future). You can download the extension from Sun Microsystems. Mac users must download it from Apple instead. How do I extract data from images?Real-world values (e.g. chlorophyll concentration) can be extracted from the imagery by downloading the black and white GIFS or 8bit files and applying the appropriate conversion equation with the slope and intercept values found in the info file (seen when you display an image). Most of the products have a linear scaling applied (nLw_xxx, La_xxx, tau_865 and eps_87) and the conversion equation will be: value = (DN * slope) + intercept For other products (e.g. nasa_chlor_a, K_490) which are log scaled the conversion equation will be: value = 10^[(DN * slope) + log10(intercept)]
DN is the Digital Number within the 8bit or GIF file, which will be in the range 0 to 255. We use 0 (black) for pixels with no data and 255 (white) for annotation. Please use the 'nasa_chlor_a' product (rather than 'chlor_a') for extracting chlorophyll values; an 8bit version is provided for this purpose. If you have a real-world value and wish to know what digital number it would be represented by in the image, here are the reverse equations for linear and log scaling respectively (then round to the nearest integer): DN = (value - intercept) / slope DN = [log10(value) - log10(intercept)] / slope
NB: In the intercept column of the table below, where the scale is logarithmic, the values shown have already had their base-10 logarithm computed. Therefore, in the equation substitute the entire 'log10(intercept)' term for the value in the table. The following table lists the scaling type and the scaling parameters normally used for the common products. However you should always check the .info file corresponding to the image, as these values may be different for particular areas.
The images we produce are in Mercator projection and there are a set of fairly simple formulae for converting latitude/longitude (lat/lon) positions to x/y pixel co-ordinates. Calculate X position. FractX = (lon - minlon) / (maxlon - minlon) x = (cols - 1) * FractX Calculate Y position. Ymin = ln (tan (DEGTORAD * (45.0 + (minlat / 2.0)))) Ymax = ln (tan (DEGTORAD * (45.0 + (maxlat / 2.0)))) Yint = ln (tan (DEGTORAD * (45.0 + (lat / 2.0)))) FractY = (Yint - YMin) / (YMax - YMin) y = (rows - 1) * (1.0 - FractY) The maximum/minimum latitude/longitude values and sizes are given when the images are viewed. For converting from x/y pixel co-ordinates on a Mercator projection image to latitude/longitude (lat/lon) positions use: Calculate longitude. lonfract = x / (cols - 1) lon = minlon + (lonfract * (maxlon - minlon)) Calculate latitude. latfract = 1.0 - (y / (rows - 1)) Ymin = ln (tan (DEGTORAD * (45.0 + (minlat / 2.0)))) Ymax = ln (tan (DEGTORAD * (45.0 + (maxlat / 2.0)))) Yint = Ymin + (latfract * (Ymax - Ymin)) lat = 2.0 * (RADTODEG * (arctan (exp (Yint))) - 45.0) The maximum/minimum latitude/longitude values and sizes are given when the images are viewed. Here is some information about the format of raw 8bit data files and how to use them. Specific algorithms:This consists of two products, NDVI and EVI. For more information, see the MODIS Land Team website at http://modis-land.gsfc.nasa.gov/ or for algorithm details, see the ATBD at http://modis.gsfc.nasa.gov/data/atbd/atbd_mod13.pdf NDVI has the usual definition of (NIR-RED)/(NIR+RED), while EVI is defined as 2(NIR-RED)/(L+NIR+C1*RED+c2*BLUE), where L, C1 and C2 are parameters. This is claimed to have improved resistance to effects of atmosphere and background, e.g. soil. Both have a practical range of 0 (no vegetation) to 1 (maximum cover). We have implemented NASA's vegetation index retrieval package, and performed some basic validation of our results against those produced by NASA. The scattergram shows an example NDVI comparison for a scene with high NDVI variability. The small differences seen are probably due to differences between software versions, or between instrument calibration files. ![]() At the moment no cloud clearing is possible on individual images, but where images overlap in composites we select the pixel with the highest vegetation index, which is more likely to be cloud free. Below is an example image of MODIS NDVI: This also consists of two products, the TOA vegetation index and the BOA vegetation index. For more information visit the Meris website at http://envisat.esa.int/instruments/meris/ or for algorithm details see the ATBDs at http://envisat.esa.int/instruments/meris/atbd/atbd_mgvi_jrc.pdf and http://envisat.esa.int/instruments/meris/atbd/atbd_2_22.pdf The TOA vegetation index, or Meris Global Vegetation Index (MGVI) is similar to NDVI but claims a better correlation with FAPAR, the fraction of absorbed photosynthetically active radiation, an in situ measure of vegetation activity. It also has a practical range of 0 to 1. The BOA vegetation index, or Meris Terrestrial Chlorophyll Index (MTCI) aims to represent canopy chlorophyll content. Hence it does not have a theoretical maximum value, but practical values range from 0 to about 4.2. Cloud clearing is integrated into these algorithms. Below are example images of MERIS TOA and BOA vegetation index: This is a published case 2 waters chlorophyll-a estimation algorithm. Reference: These measurements are derived using the PML Inherent Optical Property model (Smyth, T.J., Moore, G.F., Hirata, T. & Aiken, J. (2006) Semianalytical model for the derivation of ocean color inherent optical properties: description, implementation, and performance assessment. Applied Optics, 45(31), 8116-8131. Download paper (PDF 3 MB) Further information:To do so please include : Our privacy policy is detailed here. Our copyright status is covered in the terms of use here. AVHRR HRPT satellite images are obtained via a fast Internet link from Dundee Satellite Receiving Station, by special arrangement. The SST equation coefficients were obtained from NOAA Polar Orbiter Data User's Guide, NOAA KLM User's Guide, NOAA Satellite Information System, and various other sources. Thiermann V, Ruprecht E. A method for the detection of clouds using AVHRR infrared observations. Int. J. Remote Sensing 13(10):1829-1841, 1992. Saunders RW, Kriebel KT. An improved method for detecting clear sky and cloudy radiances from AVHRR data. Int. J. Remote Sensing 9(1):123-150, 1988. Roozekrans JN, Prangsma GJ. Processing and application of digital AVHRR imagery for land and sea surfaces. Royal Netherlands Meteorological Institute (KNMI), 1988. Dalu G. Satellite remote sensing of atmospheric water vapour. Int. J. Remote Sensing 7(9):1089-1097, 1986. McClain, C.R. 1997. 'SeaWiFS Bio-optical Mini-workshop (SeaBAM) Overview' or SeaBAM WWW page. O'Reilly, J.E. and co-authors, 2000: "Ocean color chlorophyll a algorithms for SeaWiFS, OC2, and OC4: Version 4." In: J.E. O'Reilly and co-authors, SeaWiFS Postlaunch Calibration and Validation Analyses, Part 3. NASA Tech. Memo. 2000-206892, Vol. 11, S.B. Hooker and E.R. Firestone, Eds., NASA Goddard Space Flight Center, Greenbelt, Maryland, 9-23. |