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What is the Triangular shaped Structure in STEREO Behind HI2?

Triangular shaped object in STEREO data explained

Some people have noticed a strange triangular or diamond-shape "object" entering the field-of-view of the HI2 telescope on STEREO Behind around December 26, 2011. You can see the feature in question in this movie moving from right-to-left, just above the trapezoidal occulter on the right side of the image, and more clearly in this close-up movie . What is this?

The answer lies on the exact opposite side of the image. At the same time as this strange-looking feature starts being visible, the very bright planet Venus enters the HI2-B field-of-view from the lower left. Notice that Venus and the feature stay in step almost exactly opposite each other across the middle of the detector. This is not a coincidence. The strange looking geometrical "object" is actually an internal reflection of the planet Venus within the telescope optics. This effect has been seen many times before. Here's a particularly striking example of internal reflections caused by the planet Earth as seen early in the STEREO mission, taken from our image artifacts pages.

Earth is also visible in the December 2011 movie, but is not as bright as Venus. It is the stationary object to the center left. As an added bonus, the tail of Comet Lovejoy can be seen entering from the left towards the end of the movie, just below Venus. Here is a diagram showing the location of the various features in the image:

Here are the movies showing this artifact in late December 2011:


Stereo behind HI2 Dec 29-30 2011 (part 1)

 
Link
Observations:
Triangle/Pyramid shaped structure, not solid. Looks like made from tubes
Dimensional
Tumbling from right to left


Close-Up



For images:
Search for STEREO Images: http:// stereo-ssc.nascom.nasa.gov/ cgi-bin/images
Settings:
Telescope: Behind H12
Resolution: 1024x1024
Display: Images
Dates: 20111229 End: 20111230
Hit Search
For Slideshow/Movie:
Search for STEREO Images: http:// stereo-ssc.nascom.nasa.gov/ cgi-bin/images
Settings:
Telescope: Behind H12
Resolution: 1024x1024
Display: Slideshow
Dates: 20111229 End: 20111230
Hit Search

ps. images blanked out after Dec 30 2011 22:10


Stereo behind HI2 dec 29 2011 - Jan 10 2012 (part 2)


Note: Could it be some sort of Boom System?
http://www.compositesworld.com/articles/self-deployable-composite-satellite-boom


used 4 radio telescopes etc

 

The same object appeared on STEREO Behind HI2 in 2007

Click an image to enlarge >>





Another strange object was captured on STEREO Ahead HI2 on Oct 25 2011
STEREO Ahead HI2 Oct 25 2011

For images:
Search for STEREO Images: http:// stereo-ssc.nascom.nasa.gov/ cgi-bin/images
Settings:
Telescope: Behind H12
Resolution: 1024x1024
Display: Images
Dates: 20111025 End: 20111026
Hit Search
For Slideshow/Movie:
Search for STEREO Images: http:// stereo-ssc.nascom.nasa.gov/ cgi-bin/images
Settings:
Telescope: Behind H12
Resolution: 1024x1024
Display: Slideshow
Dates: 20111025 End: 20111026
Hit Search



Positions of STEREO A (Ahead) and B (Behind) on Dec 30 2011 10:15

 
STEREO-B
 
Earth
 
STEREO-A
Heliocentric distance (AU)
Semidiameter (arcsec)
1.073090 894.266
 
0.983371
975.856
 
0.962989
996.510
HCI longitude
HCI latitude
271.698
7.305
 
22.261
-2.762
 
129.716
-5.610
Carrington longitude
Carrington rotation number
27.865
2118.923
 
138.428
2118.615
 
245.884
2118.317
Heliographic (HEEQ) longitude
Heliographic (HEEQ) latitude
-110.563
7.305
 
0.000
-2.762
 
107.455
-5.610
HAE longitude
347.450
 
98.189
 
205.254
Earth Ecliptic (HEE) longitude
Earth Ecliptic (HEE) latitude
-110.739
0.056
 
-0.000
0.000
 
107.066
-0.020
Roll from ecliptic north
Roll from solar north
-0.019
0.196
 
 
-0.008
-4.634
Light travel time to Earth (min)
14.080
13.019
Separation angle with Earth
Separation angle A with B
110.739

142.195
 
107.066


There are five imaging instruments on each STEREO spacecraft. They form STEREO's SECCHI imaging suite.

Together they image all the way from the Sun to the orbit of Earth - the first time this has been done with a single spacecraft. This is such a distance across the sky that it is difficult to depict on a flat screen.

The image above shows the fields of view (FOV) of the three sun centered imagers:

  • EUVI - Shows the Sun in extreme UV light out to 1.7 times the Sun's radius
  • Cor1 - Visible light coronagraph which observes from 1.5 to 4 solar radii
  • Cor2 - visible light coronagraph which observes out to 15 solar radii


In this depiction Earth's orbit is on the left and the Sun is on the right.

In addition to the data from three sun-centered imagers show above, here we also see data from the two Heliocentric Imagers, visible light imagers which are pointed away from the Sun:

  • HI1 - Observes visible light from the outer part of Cor2's field of view to about a third of the distance to Earth's orbit
  • HI2 - Completes the Sun-Earth view by extending the view to Earth's orbit

The illustration only shows the fields of view of the Ahead spacecraft. The Behind spacecraft observes the area between the Sun and Earth from the other direction, so that between them we see 180 degrees of sky.

Source: STEREO/SECCHI Imagers: Fields of View
Here's an image from the HI2-B telescope which shows a number of interesting internal reflections.
Source
Link | Source
The brightest object in the field is our own planet Earth, which is responsible for all the reflection effects. Also visible is the Moon, and the planet Mars.
Internal reflections of the planet Earth, as seen in the HI2-B telescope on May 5, 2007.



Image artifacts - Beacon data

STEREO has two separate telemetry streams coming down from each spacecraft, the space weather beacon telemetry, and the science recorder playback telemetry. The beacon telemetry contains the most recent data and images, and is transmitted 24 hours per day. A volunteer network of antenna stations around the world collect as much as possible of this real-time data stream, and send it to the STEREO Science Center for processing. However, because the beacon telemetry rate is very low, the images need to be compressed by large factors, and are thus of much lower quality than the actual science data.

The science data collected by the STEREO spacecraft are written to the on-board recorder, which is then read out and transmitted to the ground during daily telemetry tracks using the NASA Deep Space Network. These data are of much higher quality than the beacon data, but take several days to reach the STEREO Science Center website. Thus, the most recent images on the STEREO Science Center browse tool will always be beacon images. These temporary beacon images are replaced with the full-quality versions as they become available, generally about 2-3 days later.

Beacon images can always be recognized by having the character " 7 " near the end of the filename, e.g. "n 7 euA", while the full resolution images will have the character " 4 " in that location.

Also check out the write-up on cosmic rays to see how the high compression factors used for the beacon data affect those artifacts.

Although the initial beacon JPEG images on the browse pages are replaced by the high resolution images as they become available, the original FITS versions of the beacon files are saved, and can be read using any of a large number of software packages , most of which are free.

Useful Links:
Planet Finder
latest SECCHI beacon images
Stereo Learning Center
Image Artifacts - Internal Reflections









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Useful Links
Observing the Sun and Planets & Anomalies Explained
 
Stereo Learning Center
Where is STEREO?
STEREO Orbit Tool
Java orbit viewer (NRL)
STEREO/SECCHI Imagers: Fields of View
Search for STEREO Images
Planet Finder
latest SECCHI beacon images
Image Artifacts - Internal Reflections

Satellite Situation Center (SSCWeb)
HelioWeb
Connections with planetary missions
Explanation of coordinate systems

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