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Select AllLimit search to the following Collections: Searching 1 of 1Clear
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David Rumsey Historical...
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MEDIA INFORMATION

 
 
 
COLLECTION NAME:
David Rumsey Historical Map Collection
mediaCollectionId
RUMSEY~8~1
David Rumsey Historical Map Collection
Collection
true
Record 
Author:
USGS Astrogeology Science Center
author
USGS Astrogeology Science Center
Author
false
Search Author
Date:
2014
date
2014
Date
false
Search Date
Short Title:
Venus Magellan Global C3-MDIR Synthetic Color Mosaic 4641m v1
short_title
Venus Magellan Global C3-MDIR Synthetic Color Mosaic 4641m v1
Short Title
false
Search Short Title
Publisher:
USGS Astrogeology Science Center
publisher
USGS Astrogeology Science Center
Publisher
false
Search Publisher
Publisher Location:
Flagstaff
publisher_location
Flagstaff
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false
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Type:
Aerial Photograph
type
Aerial Photograph
Type
false
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Reference:
Link to source image: https://astrogeolog…
reference
Link to source image:
https://astrogeology.usgs.gov/search/map/Venus/Magellan/Colorized/Venus_Magellan_C3-MDIR_Colorized_Global_Mosaic_4641m
Reference
false
Search Reference
Region:
Venus
region
Venus
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Search Region
Subject:
Celestial
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Celestial
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Search Subject
Full Title:
Venus Magellan Global C3-MDIR Synthetic Color Mosaic 4641m v1
full_title
Venus Magellan Global C3-MDIR Synthetic Color Mosaic 4641m v1
Full Title
false
Search Full Title
List No:
10606.000
list_no
10606.000
List No
false
Search List No
Publication Author:
USGS Astrogeology Science Center
publication_author
USGS Astrogeology Science Center
Publication Author
false
Search Publication Author
Pub Date:
2014
pub_date
2014
Pub Date
false
Search Pub Date
Pub Title:
Venus Magellan Global C3-MDIR Synthetic Color Mosaic 4641m v1
pub_title
Venus Magellan Global C3-MDIR Synthetic Color Mosaic 4641m v1
Pub Title
false
Search Pub Title
Pub Note:
This synthetic colorized version of the C3-MIDR mosaic was developed to simulate
the surface of Venus. This mosaic was created from the Magellan Full resolution
Basic Image Data Records (F-BIDRs), the highest resolution radar images of the
Venus surface (~75 meters per pixel [m]). To make this product, the F-BIDR is
assembled into Full-Resolution Mosaicked Image Data Records (F-MIDRs) which are
then averaged in successive operations resulting in each pixel being the average
of nine pixels resulting in compressed BIDR or C-BIDR. The resulting C-BIDR are
then mosaicked into 8192 x 8192 arrays called C1-MIDR (Compressed Once -
Mosaicked Image Data Record) which are then further compressed into C2- and
C3-MIDR. The original Magellan Compressed Mosaicked Image Data Record (C3-MIDR)
archive contains three times compressed mosaics of image swaths (C-BIDRs) at a
resolution of 2025 m/pixel. C3-MIDRs consist of mosaics generated by computing
3x3 pixel arithmetic moving averages from the C2-MIDRs. C3-MIDRs, with their
2.025 km pixel widths, are designed to cover the planet at reasonably high
resolution and high signal to noise ratio. (Ford et al., 1993). Mission and
Instrument Information: The Magellan Mission to Venus launched on May 4, 1989 on
board the Space Shuttle Atlantis. The spacecraft arrived at Venus on August
10th, 1990 and was inserted into a near-polar elliptical orbit. The primary
mission requirements were to map at least 70% of the surface at a resolution
better than 300 meters/pixel and to determine the global relief at such a
resolution as to facilitate detailed analysis of tectonic, volcanic, eolian, and
impact features. Magellan successfully completed four mapping cycles at Venus.
The first mapping cycle lasted from mid-September 1990 to mid-May 1991 focused
on fulfilling the primary mission requirements. The second mapping cycle was
from mid-May 1991 to mid-January 1992 and was dedicated to filing in gaps in the
cycle 1 coverage and obtaining coverage of the south polar region; this cycle
resulted in 54% of surfaced coverage and increased the cumulative coverage of
the mission to 96%. Cycle 3 was from mid-January to mid-September 1992 and
focused on acquiring stereo image coverage; this cycle resulted in about 21%
surface coverage and increased total surface coverage to 98%. Cycle 4 was
dedicated to gravity observations and as such did not add to the cumulative
coverage of imagery taken by the spacecraft (Ford et al., 1993).
pub_note
This synthetic colorized version of the C3-MIDR mosaic was developed to simulate
the surface of Venus. This mosaic was created from the Magellan Full resolution
Basic Image Data Records (F-BIDRs), the highest resolution radar images of the
Venus surface (~75 meters per pixel [m]). To make this product, the F-BIDR is
assembled into Full-Resolution Mosaicked Image Data Records (F-MIDRs) which are
then averaged in successive operations resulting in each pixel being the average
of nine pixels resulting in compressed BIDR or C-BIDR. The resulting C-BIDR are
then mosaicked into 8192 x 8192 arrays called C1-MIDR (Compressed Once -
Mosaicked Image Data Record) which are then further compressed into C2- and
C3-MIDR. The original Magellan Compressed Mosaicked Image Data Record (C3-MIDR)
archive contains three times compressed mosaics of image swaths (C-BIDRs) at a
resolution of 2025 m/pixel. C3-MIDRs consist of mosaics generated by computing
3x3 pixel arithmetic moving averages from the C2-MIDRs. C3-MIDRs, with their
2.025 km pixel widths, are designed to cover the planet at reasonably high
resolution and high signal to noise ratio. (Ford et al., 1993). Mission and
Instrument Information: The Magellan Mission to Venus launched on May 4, 1989 on
board the Space Shuttle Atlantis. The spacecraft arrived at Venus on August
10th, 1990 and was inserted into a near-polar elliptical orbit. The primary
mission requirements were to map at least 70% of the surface at a resolution
better than 300 meters/pixel and to determine the global relief at such a
resolution as to facilitate detailed analysis of tectonic, volcanic, eolian, and
impact features. Magellan successfully completed four mapping cycles at Venus.
The first mapping cycle lasted from mid-September 1990 to mid-May 1991 focused
on fulfilling the primary mission requirements. The second mapping cycle was
from mid-May 1991 to mid-January 1992 and was dedicated to filing in gaps in the
cycle 1 coverage and obtaining coverage of the south polar region; this cycle
resulted in 54% of surfaced coverage and increased the cumulative coverage of
the mission to 96%. Cycle 3 was from mid-January to mid-September 1992 and
focused on acquiring stereo image coverage; this cycle resulted in about 21%
surface coverage and increased total surface coverage to 98%. Cycle 4 was
dedicated to gravity observations and as such did not add to the cumulative
coverage of imagery taken by the spacecraft (Ford et al., 1993).
Pub Note
false
Search Pub Note
Pub List No:
10606.000
pub_list_no
10606.000
Pub List No
false
Search Pub List No
Pub Type:
Aerial Photograph
pub_type
Aerial Photograph
Pub Type
false
Search Pub Type
Image No:
10606000.jp2
image_no
10606000.jp2
Image No
false
Search Image No
Download 1:
Full Image Download…
fullsidurl
<a href=https://www.davidrumsey.com/rumsey/download.pl?image=/185/10606000.jp2
target=_blank>Full Image Download in JP2 Format</a>
Download 1
false
Search Download 1
Download 2:
GeoViewer for JP2 a…
mrsidsoftwareurl
<a href=https://www.extensis.com/support/geoviewer-9 target=_blank >GeoViewer
for JP2 and SID files</a>
Download 2
false
Search Download 2
Authors:
USGS Astrogeology Science Center
author_thumbnail_label
USGS Astrogeology Science Center
Authors
false
Search Authors
Text on Maps:  




VENUS MAGELLAN GLOBAL C3-MDIR SYNTHETIC COLOR MOSAIC 4641M V1

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