CLEM UVVIS Experiment Data Record (EDR)
EDR – Experiment Data Record
Instrument: Ultraviolet/Visible Camera
PDS Data Set ID: CLEM1-L/E/Y-U-2-EDR-V1.0DOI: 10.17189/1520261
For more information about UVVIS EDR products, see the EDR Image SIS.
The Ultraviolet/Visible camera (UVVIS) Experiment Data Record (EDR) data products are raw images. Data have been depacketized and reformatted, but are otherwise “raw”. Raw data contain the geometric and radiometric characteristics of unprocessed and unrectified data. To make full utilization of the data, it is necessary to perform radiometric and geometric processing on the data products.
UVVIS is used for science observations. It has a filter wheel that allow images to be acquired under six spectral filters at wavelengths of 415 nm, 750 nm, 900 nm, 950 nm, 1000 nm, and 650 nm (broadband). Each HIRES EDR image is 288 lines by 384 samples.
UVVIS EDR lunar mapping phase products have the following file names:
LUfxxxxy.nnn
where:
f = filter wheel position = A, B, C, D, E, F, or “_”
xxxx = frame number within revolution
y = latitude bin for lunar mapping observations; signifies a latitude range on the lunar surface where the observation was made (see table below)
rrr = 3-digit orbit number
UVVIS EDR non-lunar mapping phase products have the following file names:
mUfxxxxy.nnn
where:
m = Mission Phase
A = Earth phasing loop A
B = Earth phasing loop B
f = filter wheel position = A, B, C, D, E, F, or “_”
xxxx = frame sequence number within a download dump of the spacecraft’s solid state recorder; the solid state recorder, holding acquired images, is periodically downloaded to Earth; images are number sequentially by time of observation
y = alpha character; each 100 sequential images of a camera are assigned an alpha character A-Z
rrr = memory download sequence number; incremented by one each time a download is made of the solid state data recorder within a mission phase
In ODE, EDR products have the following product IDs:
LUFXXXXY.NNN
MUFXXXXY.NNN
Latitude bin for lunar mapping observations and alpha character for non-lunar mapping phase:
Character |
Lunar Mapping Latitude Bins |
Non-Lunar Mapping Phasing Loop |
A |
-90 to -80 |
A or B |
B |
-80 to -70 |
A or B |
C |
-70 to -60 |
A or B |
D |
-60 to -50 |
A or B |
E |
-50 to -40 |
A or B |
F |
-40 to -30 |
A or B |
G |
-30 to -20 |
A or B |
H |
-20 to -10 |
A or B |
I |
-10 to 0 |
A or B |
J |
0 to 10 |
A or B |
K |
10 to 20 |
A or B |
L |
20 to 30 |
A or B |
M |
30 to 40 |
A or B |
N |
40 to 50 |
B only |
O |
50 to 60 |
B only |
P |
60 to 70 |
B only |
Q |
70 to 80 |
N/A |
R |
80 to 90 |
N/A |
S |
“unknown” targets |
N/A |
T |
Earth observations prior to systematic mapping |
N/A |
U |
Sky observations prior to systematic mapping |
N/A |
V |
Lunar observations prior to systematic mapping |
N/A |
W |
Sky observations after systematic mapping |
N/A |
Y |
Earth observations after systematic mapping |
N/A |
Z |
Lunar observations after systematic mapping |
N/A |