List of Analyzed UVI Images



Date

Time (UT)

Comment

Analysis¹

Overview Plot

19-20 May, 1996 (96140-96141)

17:30-02:30

ISTP "Theory" event

A

hemispheric power
raw data 1729-2053
raw data 2058-2355
raw data 0005-0330
energy flux

27 May, 1996 (96148)

16:30-22:15

ISTP Southern hemisphere event (POLAR perigee)

A

Summary raw data
energy flux

29 May, 1996 (96150)

2:00-7:10

Dim aurora, hemispheric power is below 15 GW

D,F² (samples)


N/A

10 December, 1996 (96345)

0:00-0:03

VIS-UVI comparison

D,F,E (samples)

N/A

1-2 January, 1997 (97001-97002)


Gap in the oval

none

Summary raw data

9 January, 1997 (97009)

7:00-11:00

Substorm before the CME arrives

A

Summary raw data
hemispheric power

10 January, 1997 (97010)

0:00-5:45 10:00-23:00

Large CME event

A

Summary raw data
hemispheric power
energy flux

11 January, 1997 (97011)

6:00-16:06

Large CME event

A

Summary raw data
hemispheric power
energy flux

12 January, 1997 (97012)

6:40-10:00

Large CME event

A

Summary raw data
hemispheric power

18 January, 1997 (97018)

1:00-3:00

LBH-l only²

D,F

hemispheric power

9 April, 1997 (97099)

5:10-9:56 13:50-16:33

UARC campaign

A

Summary raw data
hemispheric power

10 April, 1997 (97100)

20:00-23:59

UARC campaign

A

Summary raw data
hemispheric power
energy flux

15 May, 1997 (97135)

7:34-14:35

Dayside Aurora

A

Summary raw data

7 August, 1997 (97219)

0:00-0:40


D,F,E

N/A

3 October, 1997 (97276)

10:00-11:00

High spatial resolution

A

N/A

1 May, 1998 (98121)

0:01-2:25 13:35-20:02

Gaps in the analysis

A

hemispheric power

4 May, 1998 (98124)

0:00-1:01 8:30-18:29


A

hemispheric power

25 June, 1998 (98176)

12:50-17:40

Dim aurora, gaps in the analysis

A

N/A

26 June, 1998 (98177)

4:12-9:13


A

N/A

8 March, 1999 (99067)

14:00-14:15


D,F,E

N/A

22 October, 1999 (99295)

6:31-12:30

LBH-l only²

D,F (samples)

N/A

30 January, 2000 (00030)

1:30-1:40

LBH-l only²

D,F

N/A

¹Key for analysis: D: dayglow removal; F: energy flux; E: mean energy; C: conductance; A: AMIE input file generated (implies D, F, E, and C)

²When the UVI operating mode does not provide for alternating LBH-long and LBH-short filters, we can only get the energy flux.





Last modified 3/19/01 by Dirk Lummerzheim