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Solar Bulletin, June 2003
Solar Bulletin |
| THE AMERICAN ASSOCIATION OF VARIABLE STAR OBSERVERS - SOLAR COMMITTEE |
Carl E. Feehrer, Editor
9 Gleason Rd.
Bedford, MA 01730 | Email: cfeehrer@hotmail.com
ISSN 0271-8480 |
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| Volume 59 Number 6 | June 2003 |
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Table I. Mean Sunspot Numbers for June 2003 [boldface = maximum, minimum] | Table II. June Observers |
| Day |
N |
Raw |
s.d. |
Ra |
s.d. |
s.e. |
| 1 |
47 |
53 |
3.0 |
40 |
1.9 |
0.28 |
| 2 |
45 |
55 |
2.8 |
40 |
1.3 |
0.19 |
| 3 |
40 |
55 |
2.3 |
42 |
1.1 |
0.17 |
| 4 |
38 |
67 |
3.3 |
52 |
1.6 |
0.26 |
| 5 |
40 |
85 |
4.3 |
62 |
2.3 |
0.36 |
| 6 |
50 |
122 |
5.9 |
88 |
2.6 |
0.37 |
| 7 |
40 |
136 |
6.8 |
103 |
2.1 |
0.33 |
| 8 |
44 |
134 |
7.4 |
100 |
2.3 |
0.35 |
| 9 |
49 |
150 |
8.8 |
112 |
3.8 |
0.54 |
| 10 |
45 |
148 |
8.2 |
110 |
3.3 |
0.49 |
| 11 |
44 |
163 |
7.3 |
121 |
3.3 |
0.50 |
| 12 |
40 |
161 |
6.6 |
120 |
2.7 |
0.43 |
| 13 |
43 |
131 |
6.2 |
100 |
3.2 |
0.49 |
| 14 |
40 |
96 |
5.8 |
70 |
2.3 |
0.36 |
| 15 |
41 |
64 |
4.7 |
49 |
2.5 |
0.39 |
| 16 |
52 |
73 |
3.4 |
56 |
1.6 |
0.22 |
| 17 |
44 |
74 |
3.9 |
56 |
1.8 |
0.27 |
| 18 |
45 |
86 |
3.5 |
66 |
1.6 |
0.24 |
| 19 |
46 |
101 |
4.7 |
76 |
1.9 |
0.28 |
| 20 |
44 |
105 |
5.5 |
78 |
2.3 |
0.35 |
| 21 |
45 |
93 |
5.2 |
69 |
2.1 |
0.31 |
| 22 |
46 |
85 |
4.3 |
65 |
2.2 |
0.32 |
| 23 |
45 |
94 |
4.5 |
69 |
2.1 |
0.31 |
| 24 |
53 |
98 |
4.4 |
74 |
2.1 |
0.29 |
| 25 |
44 |
107 |
4.3 |
79 |
1.7 |
0.26 |
| 26 |
48 |
114 |
5.1 |
84 |
2.5 |
0.36 |
| 27 |
46 |
124 |
4.5 |
93 |
2.2 |
0.32 |
| 28 |
46 |
125 |
4.4 |
95 |
1.6 |
0.24 |
| 29 |
46 |
126 |
5.2 |
92 |
2.0 |
0.29 |
| 30 |
39 |
117 |
5.8 |
85 |
2.3 |
0.37 |
| 31 |
--- |
--- |
--- |
--- |
--- |
--- |
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Means: | 44.5 | 104.7 | | 78.2 | | |
No. of Observations: 1335
No. of Observers: 79
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Reporting Addresses |
Sunspot Reports -- email: solar@aavso.org
- postal mail: AAVSO, 25 Birch St. Cambridge, MA 02138
- FAX (AAVSO): (617) 354-0665
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SID Solar Flare Reports -- email: noatak@aol.com
- postal mail: Mike Hill
114 Prospect St. Marlboro, MA 01752
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|
| 10 |
AAP |
P.Abbott |
| 27 |
ARAG |
G.Araujo |
| 28 |
ATON |
A.Attanasio |
| 15 |
BARH |
H.Barnes |
| 20 |
BATR |
R.Battaiola |
| 16 |
BERJ |
J.Berdejo |
| 9 |
BLAJ |
J.Blackwell |
| 19 |
BMF |
M.Boschat |
| 25 |
BOJP |
P.Bojda |
| 27 |
BRAB |
B.Branchett |
| 14 |
BRAD |
D.Branchett |
| 23 |
BRAR |
R.Branch |
| 30 |
BROB |
R.Brown |
| 2 |
BURS |
S.Burgess |
| 23 |
BWJ |
J.Bohdanowicz |
| 10 |
CAMP |
P.Campbell |
| 17 |
CARJ |
J.Carlson |
| 30 |
CHAG |
G.Morales |
| 30 |
CKB |
B.Cudnik |
| 17 |
CLZ |
C.Laurent |
| 17 |
COMT |
T.Compton |
| 29 |
CORA |
A.Coroas |
| 25 |
CR |
T.Cragg |
| 8 |
CVJ |
J.Carvajal |
| 25 |
DEJV |
J.van Delft |
| 4 |
DELS |
S.Delaney |
| 15 |
DEMF |
F.Dempsey |
| 25 |
DRAJ |
J.Dragesco |
| 27 |
DUBF |
F.DuBois |
| 10 |
FEEC |
C.Feehrer |
| 18 |
FERJ |
J.Fernandes |
| 6 |
FLET |
T.Fleming |
| 24 |
GIOR |
R.Giovanoni |
| 15 |
GOEM |
M.Goetz |
| 7 |
GOLA |
A.Golovin |
| 11 |
GOTS |
S.Gottschalk |
| 7 |
HALB |
B.Halls |
| 7 |
HAYK |
K.Hay |
| 13 |
HRUT |
T.Hrutkay |
| 17 |
JAMD |
D.James |
| 6 |
JEFT |
T.Jeffrey |
| 4 |
JENS |
S.Jenner |
| 22 |
KAPJ |
J.Kaplan |
| 15 |
KHAR |
R.Khan |
| 21 |
KNJS |
J&S Knight |
| 3 |
KROL |
L.Krozel |
| 1 |
KUZM |
M.Kuzmin |
| 15 |
LARJ |
J.Larriba |
| 19 |
LERM |
M.Lerman |
| 21 |
LEVM |
M.Leventhal |
| 10 |
LUBT |
T.Lubbers |
| 22 |
MALK |
K.Malde |
| 24 |
MARJ |
J.Maranon |
| 18 |
MCE |
E.Mochizuki |
| 12 |
MILJ |
J.Miller |
| 20 |
MMI |
M.Moeller |
| 14 |
OBSO |
IPS Observatory |
| 8 |
PARN |
N.Parker |
| 22 |
RICE |
E.Richardson |
| 16 |
RITA |
A.Ritchie |
| 25 |
SCGL |
G.Schott |
| 6 |
SCHG |
G.Scholl |
| 2 |
SDP |
D.Sharples |
| 12 |
SIMC |
C.Simpson |
| 30 |
STAB |
B.Gordon-States |
| 6 |
STEF |
G.Stefanopoulis |
| 26 |
STEM |
G.Stemmler |
| 29 |
STQ |
N.Stoikidis |
| 14 |
SUZM |
M.Suzuki |
| 14 |
SZAK |
K.Szatkowski |
| 26 |
SZUM |
M.Szulc |
| 25 |
TESD |
D.Teske |
| 20 |
THR |
R.Thompson |
| 9 |
TJV |
J.Temprano |
| 21 |
VARG |
A.Vargas |
| 23 |
VIDD |
D.Vidican |
| 18 |
WILW |
W.Wilson |
| 30 |
YESH |
H.Yesilyaprak |
| 4 |
ZDM |
D.Zhdanok |
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| Table III. Means of Raw Group Counts (RG) and Ratios of Spots to Groups (S:G) in June 2003 |
| Day |
RG |
S:G |
Day |
RG |
S:G |
Day |
RG |
S:G |
Day |
RG |
S:G |
| 1 |
3.4 |
5.6 |
9 |
5.4 |
17.8 |
17 |
4.8 |
5.4 |
25 |
6.6 |
6.2 |
| 2 |
3.4 |
6.2 |
10 |
5.1 |
19.0 |
18 |
5.3 |
6.2 |
26 |
7.4 |
5.4 |
| 3 |
3.3 |
6.7 |
11 |
5.6 |
19.1 |
19 |
5.4 |
8.7 |
27 |
8.2 |
5.1 |
| 4 |
4.2 |
6.0 |
12 |
6.1 |
16.4 |
20 |
4.8 |
11.9 |
28 |
7.9 |
5.8 |
| 5 |
5.2 |
6.4 |
13 |
6.1 |
11.5 |
21 |
4.0 |
13.2 |
29 |
7.9 |
6.0 |
| 6 |
6.8 |
7.9 |
14 |
5.3 |
8.1 |
22 |
4.0 |
11.3 |
30 |
6.9 |
7.0 |
| 7 |
6.8 |
10.0 |
15 |
4.0 |
6.0 |
23 |
5.0 |
8.8 |
31 |
--- |
--- |
| 8 |
5.8 |
13.1 |
16 |
4.6 |
5.9 |
24 |
5.9 |
6.6 |
Mn. |
5.5 |
9.1 |
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Click image to enlarge. Fig.1. 10 cm Solar Flux and Comparison of Ri (provisional) and Ra Estimates for June 2003 (r=0.980).
(Ri Source: http://sidc..oma.be/index.php3)
(10cm Source: http://www.drao.nrc.ca/icarus) |
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Click image to enlarge. Fig.2 Maximum, Mean, and Minimum Ra Values for Each Month from January 2001 to Present. |
Michael Hill, SID Analyst
114 Prospect St
Marlborough, MA 01752 USA
noatak@aol.com |
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Sudden Ionospheric Disturbances (SID) Recorded During June 2003
| (Analysis performed by Michael Hill, SID Analyst) |
| Date |
Max |
Imp |
Date |
Max |
Imp |
Date |
Max |
Imp |
| 030601 |
0711 |
2 |
030609 |
2113 |
1 |
030612 |
0900 |
1- |
| 030601 |
0751 |
1 |
030609 |
2137 |
1+ |
030612 |
1006 |
1 |
| 030601 |
0905 |
2 |
030610 |
0001 |
2+ |
030612 |
1027 |
1 |
| 030601 |
1251 |
2 |
030610 |
0837 |
1+ |
030612 |
1148 |
2 |
| 030601 |
1259 |
2+ |
030610 |
1104 |
2+ |
030612 |
1407 |
2 |
| 030601 |
1653 |
2 |
030610 |
1113 |
2+ |
030612 |
1712 |
1+ |
| 030601 |
1729 |
1 |
030610 |
1204 |
1+ |
030612 |
2013 |
2 |
| 030601 |
2107 |
2 |
030610 |
1245 |
2+ |
030612 |
2127 |
2 |
| 030602 |
0835 |
2 |
030610 |
1254 |
2+ |
030613 |
0203 |
2 |
| 030602 |
1318 |
2 |
030610 |
1302 |
2+ |
030613 |
0435 |
2 |
| 030602 |
1543 |
2+ |
030610 |
1417 |
1 |
030613 |
0635 |
3 |
| 030602 |
1733 |
2+ |
030610 |
1435 |
2 |
030613 |
0644 |
3+ |
| 030604 |
1537 |
2+ |
030610 |
1625 |
1 |
030613 |
1452 |
2+ |
| 030606 |
1254 |
1 |
030610 |
1631 |
2 |
030613 |
1624 |
2+ |
| 030606 |
1316 |
1+ |
030610 |
1816 |
2 |
030613 |
1734 |
2+ |
| 030606 |
1359 |
1 |
030610 |
1854 |
2 |
030613 |
2033 |
2+ |
| 030606 |
1618 |
1 |
030611 |
0450 |
2 |
030614 |
0535 |
3 |
| 030606 |
1746 |
1+ |
030611 |
0553 |
2 |
030614 |
0558 |
3+ |
| 030608 |
0504 |
1 |
030611 |
0829 |
1+ |
030616 |
1201 |
2+ |
| 030608 |
0612 |
1+ |
030611 |
1101 |
2+ |
030617 |
2154 |
1+ |
| 030608 |
0700 |
1 |
030611 |
1321 |
2 |
030617 |
2253 |
2+ |
| 030608 |
0746 |
1 |
030611 |
1529 |
2 |
030621 |
1314 |
1+ |
| 030608 |
1145 |
2 |
030611 |
1630 |
2+ |
030624 |
0933 |
1+ |
| 030608 |
1610 |
2 |
030611 |
1743 |
2 |
030624 |
1024 |
1 |
| 030609 |
0908 |
1+ |
030611 |
2006 |
2 |
030625 |
1554 |
2 |
| 030609 |
1111 |
2 |
030612 |
0118 |
2 |
030628 |
0656 |
1 |
| 030609 |
1128 |
2 |
030612 |
0129 |
3+ |
030630 |
0735 |
2+ |
| 030609 |
1447 |
1 |
030612 |
0714 |
1 |
030630 |
0742 |
2+ |
| 030609 |
1633 |
1+ |
030612 |
0813 |
1- |
030630 |
0748 |
1+ |
| 030609 |
2059 |
1- |
030612 |
0833 |
1+ |
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| Importance rating: Duration | -1: <19 | 1: 19-25 | 1+: 26-32 | 2: 33-45 | 2+: 46-85 | 3: 86-125 | 3+: >125 |
| Observer |
Code |
Station(s) monitored |
| A Clerkin |
A29 |
NAA |
| J Winkler |
A50 |
NAA NPM NPR |
| D Toldo |
A52 |
NAA NWC XXX |
| J Ellerbe |
A63 |
ICV |
| A Panzer |
A83 |
NAA |
| W Moos |
A84 |
FTA |
| M Hill |
A87 |
NAA |
| L Anderson |
A91 |
NWC |
| G DiFillipo |
A93 |
DHO |
| T Poulos |
A95 |
NAA |
| J Wallace |
A97 |
NAA |
| M King |
A99 |
HWU |
| P Campbell |
A100 |
NLK |
| F Steyn |
A102 |
NAA NWC |
| L Observatory |
A107 |
DHO |
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| The events listed above meet at least one of the following criteria |
- Event reported by two or more observers within +/- 5 minutes
- Event matched to GOES-8 XRA event to within +/- 15 minutes and event time < 1000 UT
- Reported by observer with a high quality rating > 8 (scale 1-10)
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June was indeed a very unusual month in comparison to what one expects from a sun receding into solar minimum. Whereas the last number of months have shown declining activity, this past month showed a sudden spike in activity with a SID event count of 89 correlated events. This is the kind of number we were seeing back when the sun was peaking. Even more unusual was that so many of the events happened during one predominant time interval from June 6th to June 13th. During this time alone there were 3 X-Class events with one more following a few days later. There were 226 X-Ray flares recorded by the GOES-12 satellite. Of these, 4 were X-Class and 32 were M-Class. Seventeen of the M-Class events occurred on June 9th and 10th. A couple of very busy days! This burst of activity was due to sunspot region 375, a very large grouping that many of us, I'm sure, studied visually over the last month as well. This grouping is a very long lived region that has persisted for longer than the 27 day solar rotation period so has therefore been seen crossing the surface two times now. Out of the 89 correlated SID events 49 of them were 2 and 2+ events with another five long duration 3 and 3+ events. So not only did we have a lot of events we also had a lot of very energetic events.
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