| Paul Mortfield, Editor | Web: www.AAVSO.org |
| c/o AAVSO 25 Birch St. | Email: Paul@IndustrialStars.com |
| Cambridge, MA 02138 | ISSN 0271-8480 |
| Volume 62 Number 11 | November 2006 |
We continue to get sporadic solar activity, with several sunspots and flares recorded during November.
Gema Araujo took these images on November 13, 2006 in both white light and H-Alpha of active region 10923. Through her dedication, skill, and great observing location, Gema is compiling one of the most complete catalogs of (almost) daily solar drawings and photographic images. http://astrosurf.com/obsolar/
Bill Wilson has created an interesting program to calculate the length of a sunspot group from simple timings during visual observations. Its created as an Excel spreadsheet and is available at the link below. Now all we need are some big groups to measure. http://www.aavso.org/observing/programs/solar/solarsoftware.shtml
 | It is with sadness we report the passing of Alan H. Shapley on October 20 at age 87. Alan was instrumental in developing the AAVSO American Relative Sunspot Number (RA) in the mid 1940's. He was Director of the NOAA Geophysical Data Center in Boulder, Colorado from 1970 to 1981 and the son of Harvard astronomer Harlow Shapley. A fuller text of his career and his contributions to science and the arts can be viewed at: www.aavso.org/observing/programs/solar/shapley.shtml |
Sudden Ionospheric Disturbance Report
Michael Hill, SID Analyst
114 Prospect St
Marlborough, MA 01752 USA
noatak@aol.com
|  |
Sudden Ionospheric Disturbances (SID) Recorded During November 2006
(Analysis performed by Michael Hill, SID Analyst)
| Date |
Max |
Imp |
| 061105 |
0752 |
2 |
| 061105 |
1229 |
2 |
| 061106 |
1036 |
2+ |
| 061107 |
1256 |
1+ |
| 061107 |
1343 |
2+ |
| 061112 |
0738 |
1 |
| 061112 |
0946 |
1 |
| 061112 |
1047 |
1 |
| 061113 |
0647 |
1- |
| 061115 |
1859 |
1+ |
| 061118 |
0929 |
1- |
| 061129 |
1519 |
1 |
| 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 |
| D Toldo |
A52 |
NWC |
| J Mandaville |
A90 |
NPM |
| R Battaiola |
A96 |
HWU |
| J Wallace |
A97 |
NAA |
| F Steyn |
A102 |
NAA NWC |
| L Observatory |
A107 |
DHO |
| P Mortfield |
A108 |
NAA |
| M Suhovecky |
A115 |
NAA |
| K Hubal |
A117 |
NML |
| L Loudet |
A118 |
DHO |
| J Godet |
A119 |
GBZ GQD ICV |
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)
This month proved to be a bit more energetic than last with many fewer reports of "No SIDs". I'm sure many of you were happy to finally see some activity. A good reality check to be sure that the equipment really is working! There were 12 correlated SID events recorded this month. Most of them had a low importance rating as most were based on low level flare events. There were 170
X-Ray flares reported by the GOES satellite and of these all were B or C Class events. A lot of low level activity. Thanks to all that reported in. Wishing you all Happy Holidays and a Happy and Healthy New Year.
Solar Flare Summary Based on GOES-12 Data
Sunspot Data
American Relative Sunspot Numbers(Ra) for November
| Day |
N |
Raw
Mean |
Ra |
| 1 |
30 |
46 |
34 |
| 2 |
29 |
58 |
41 |
| 3 |
30 |
60 |
43 |
| 4 |
29 |
51 |
37 |
| 5 |
31 |
45 |
34 |
| 6 |
22 |
35 |
25 |
| 7 |
21 |
32 |
24 |
| 8 |
25 |
32 |
23 |
| 9 |
37 |
23 |
17 |
| 10 |
34 |
14 |
9 |
| 11 |
25 |
20 |
15 |
| 12 |
29 |
25 |
17 |
| 13 |
22 |
34 |
23 |
| 14 |
26 |
38 |
27 |
| 15 |
24 |
39 |
28 |
| 16 |
21 |
45 |
31 |
| 17 |
25 |
40 |
28 |
| 18 |
24 |
40 |
28 |
| 19 |
17 |
32 |
25 |
| 20 |
23 |
21 |
15 |
| 21 |
31 |
2 |
2 |
| 22 |
26 |
0 |
0 |
| 23 |
21 |
2 |
1 |
| 24 |
31 |
1 |
1 |
| 25 |
31 |
10 |
8 |
| 26 |
25 |
15 |
11 |
| 27 |
24 |
26 |
18 |
| 28 |
24 |
33 |
24 |
| 29 |
29 |
35 |
25 |
| 30 |
23 |
48 |
33 |
Means |
26.3 |
30.2 |
21.5 |
Total No. of Observers: 59
Total No. of Observations: 789
|
November 2006 Sunspot Observers
| AAP |
A. Abbott |
4 |
| ANGR |
R. Ang |
16 |
| ARAG |
G. Araujo |
24 |
| BARH |
H. Barnes |
12 |
| BATR |
R. Battaiola |
4 |
| BEB |
R. Berg |
3 |
| BEDJ |
J. Bedient |
1 |
| BERJ |
J. Berdejo |
9 |
| BLAJ |
J. Blackwell |
5 |
| BMF |
M. Boschat |
10 |
| BRAB |
B. Branchett |
29 |
| BRAM |
M. Bradbury |
2 |
| BRAR |
R. Branch |
30 |
| BROB |
R. Brown |
19 |
| BYG |
Y. Brovarets |
14 |
| CHAG |
G. Morales |
25 |
| CKB |
B. Cudnik |
18 |
| CLZ |
L. Corp |
8 |
| COMT |
T. Compton |
6 |
| CR |
T. Cragg |
22 |
| CVJ |
J. Carvajal |
8 |
| DEJV |
J. van Delft |
15 |
| DGP |
G. Dyck |
13 |
| DUBF |
F. Dubois |
20 |
| FERJ |
J. Fernandez |
20 |
| FLET |
T. Fleming |
23 |
| FUJK |
K. Fujimori |
22 |
| GFT |
F. Gobet |
7 |
| GOEM |
M. Goetz |
1 |
| HALB |
B. Halls |
4 |
| HAYK |
K. Hay |
5 |
| KAPJ |
J. Kaplan |
16 |
| KNJS |
J. & S. Knight |
18 |
| KQR |
R. Kinne |
8 |
| KROL |
L. Krozel |
2 |
| LARJ |
J. Larriba |
6 |
| MARE |
E. Mariani |
5 |
| MARJ |
J. Maranon |
24 |
| MCE |
E. Mochizuki |
18 |
| MCHL |
L. McHenry |
3 |
| MMI |
M. Moeller |
18 |
| OATS |
S. Oatney |
21 |
| OBSO |
IPS Observatory |
20 |
| PEKT |
R. Pektas |
18 |
| RICE |
E. C. Richardson |
15 |
| RITA |
A. Ritchie |
16 |
| SCGL |
G. Schott |
21 |
| SDP |
D. Sharples |
3 |
| SIMC |
C. Simpson |
5 |
| STEM |
G. Stemmler |
13 |
| STQ |
N. Stoikidis |
23 |
| SUZM |
M. Suzuki |
23 |
| SZUM |
M. Szulc |
14 |
| TESD |
D. Teske |
19 |
| TJV |
J. Temprano |
6 |
| URBP |
P. Urbanski |
12 |
| VARG |
A. Vargas |
22 |
| WILW |
W. Wilson |
17 |
| WRP |
R. Wheeler |
4 |
|
|
|
Reporting addresses:
Sunspot Reports
Email: solar@aavso.org
Postal Mail: AAVSO, 25
Birch St. Cambridge, MA, 02138
Fax: 617-354-0665
SID Flare Reports
Email: noatak@aol.com
Postal Mail: Mike Hill,
114 Prospect St., Marlboro, MA, 01752
|
|
 |
10 cm Solar Flux and American Relative Sunspot Numbers (Ra) for November 2006
(10cm Source: http://www.drao.nrc.ca/icarus) |
 |
Smoothed Mean Sunspot Numbers (Rsm) from January 2000 to May 2006 (Waldmeier method). |