PACE orbit with swaths and instrument fields of view
- Visualizations by:
- Greg Shirah
- View full credits
- In the first section, PACE's orbit is shown from a global view. PACE will be in a 98-degree-inclination, sun-synchronous polar orbit with an equatorial crossing time of 1:00 pm local time. PACE's orbital period (i.e., the time it takes to complete one orbit) is 98.3 minutes at an altitude of 676.5 km.
- In second section, the camera zooms in to look at the fields of view of each of PACE's instruments:
• The Ocean Color Instrument (OCI) viewing width is 113 degrees. During each orbit on the sunlit side of the Earth, OCI will change its pointing from 20 degrees behind the spacecraft (aft) when south of the Sun's latitude to 20 degrees ahead of the spacecraft (fore) when north. This is to avoid having the instrument’s field of view look into Sun glint. OCI will change its pointing back from fore to aft on the dark side of each orbit.
• The Hyper Angular Research Polarimeter (HARP2) instrument has a viewing width of 94 degrees. HARP2 has 10 viewing angles along the orbit track for its blue, green, and near-infrared wavelength channels and 60 viewing angles for its red wavelength channel. These viewing angles vary along the direction of travel over a range of 114 degrees. The ground swath as viewed on Earth will vary in width with viewing angle.
• The Spectro-polarimeter for Planetary Exploration (SPEXone) instrument's ground swath is about 100 km wide. SPEXone has 5 different viewing angles from -50 degrees (aft) to +50 degrees (fore). Like HARP2, the ground swath as viewed on Earth will vary in width with viewing angle. - The third section shows example ground swaths for each instrument. SPEXone has a relatively narrow swath. HARP2 has a wider swath for its nadir (straight down) view. OCI has an even wider swath. At the end all 3 instruments swaths are shown at the same time.
In terms of life on Earth, color describes more than simply how features look. In many cases color serves as a proxy for biological processes. When studying ocean biology, colors count in a big way.
The PACE mission has been conceived principally as a way to measure ocean color for assessing large scale ocean health. These measurements will provide data to determine the distribution of phytoplankton, tiny plants and algae that sustain the marine food web. A simple way to think about this is the more “green” that’s visible from space, the more prevalent are plant cells containing chlorophyll, an essential green pigment responsible for energy-producing photosynthesis in plants. Phytoplankton populations are fundamental to understanding the overall health of the ocean food web, as well as a wide range of related processes.
PACE will be able to see other colors too—a broad range of color, in fact, stretching beyond the bounds of visible light into both ultraviolet as well as infrared. PACE will also be able to make measurements of aerosols in the atmosphere, essential for scientists to improve our understanding of and our ability to forecast weather and climate.
PACE continues a more than 20 year legacy of ocean color measurements, providing the scientific community with a long time series of data. That legacy enables better assessments of long term trends about complex processes on Earth.
PACE will be able to see other colors too—a broad range of color, in fact, stretching beyond the bounds of visible light into both ultraviolet as well as infrared. PACE will also be able to make measurements of aerosols in the atmosphere, essential for scientists to improve our understanding of and our ability to forecast weather and climate.
PACE continues a more than 20-year legacy of ocean color measurements, providing the scientific community with a long time series of data. That legacy enables better assessments of long-term trends about complex processes on Earth.
Credits
Please give credit for this item to:
NASA's Scientific Visualization Studio
Visualizers
- Greg Shirah (NASA/GSFC) [Lead]
- Kel Elkins (USRA)
Scientist
- Jeremy Werdell (NASA/GSFC)
Engineer
- Fred Patt (SAIC)
Producer
- Ryan Fitzgibbons (KBRwyle)
Technical support
- Ian Jones (ADNET)
- Laurence Schuler (ADNET)
Datasets used in this visualization
SeaStar Chlorophyll Concentration (Collected with the SeaWiFS sensor)
All SeaWiFS images and data presented on this web site are for research and educational use only. All commercial use of SeaWiFS data must be coordinated with GeoEye.
Credit: NASA/Goddard Space Flight Center, The SeaWiFS Project and GeoEye, Scientific Visualization Studio. NOTE: All SeaWiFS images and data presented on this web site are for research and educational use only. All commercial use of SeaWiFS data must be coordinated with GeoEye (NOTE: In January 2013, DigitalGlobe and GeoEye combined to become one DigitalGlobe.).
Dataset can be found at: http://oceancolor.gsfc.nasa.gov/PRODUCTS/
See more visualizations using this data setSuomi NPP Chlorophyll (A.K.A. Chlorophyll Concentration) (Collected with the VIIRS sensor)
Comiso's Daily Sea Ice Concentration
Interactive Multisensor Snow and Ice Mapping System (IMS) IMS Daily Northern Hemisphere Snow and Ice Analysis (A.K.A. IMS Daily Northern Hemisphere Snow and Ice Analysis - 24 km Resolution)
SeaStar NDVI (Collected with the SeaWiFS sensor)
All SeaWiFS images and data presented on this web site are for research and educational use only. All commercial use of SeaWiFS data must be coordinated with GeoEye.
Credit: NASA/Goddard Space Flight Center, The SeaWiFS Project and GeoEye, Scientific Visualization Studio. NOTE: All SeaWiFS images and data presented on this web site are for research and educational use only. All commercial use of SeaWiFS data must be coordinated with GeoEye (NOTE: In January 2013, DigitalGlobe and GeoEye combined to become one DigitalGlobe.).
See more visualizations using this data setSuomi NPP Normalized Difference Vegetation Index (A.K.A. NDVI) (Collected with the VIIRS sensor)
Terra and Aqua NDVI (A.K.A. Normalized Difference Vegetation Index (NDVI)) (Collected with the MODIS sensor)
PACE orbit planning ephemeris (TLE) (A.K.A. PACE orbit planning ephemeris (TLE))
Credit: Fred Patt
See more visualizations using this data setNote: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.