Solobservatörerna
Wolf sunspots
number
n= k(f+10g)
g = antal
solfläcksgrupper
f = antal fläckar
w = wolf sunspots
number
Kontakt:
Observatörer
2011:
HGL = H.G.Lindberg
Refraktor
100*1000mm/120*1000mm Reflektor 254mm*1301
Projektion 160 mm,Mylarfilter, Solprisma och foto
Skultuna
2011
20110725 UT 14:00 3g 6f = 36 HGL
20110713 UT 09:15 5g 8f = 58 HGL
20110712 UT 10:50 4g 7f = 47 HGL
20110711 UT 14:30 5g 8f = 58 HGL
20110710 UT 11:15 3g 6f = 36 HGL
20110706 UT 13:00 2g 2f = 22 HGL
20110705 UT 08:30 2g 8f = 28 HGL
20110701 UT 10:50 3g 8f = 28 HGL
20110630 UT 10:50 3g 4f = 24 HGL
20110629 UT 09:40 2g 3f = 23 HGL
20110628 UT 10:00 2g 2f = 22 HGL
20110627 UT 11:00 1g 3f = 13 HGL
20110624 UT 11:00 3g 6f = 36 HGL
20110622 UT 10:30 2g 3f = 23 HGL
20110620 UT 09:30 2g 3f = 23 HGL
20110619 UT 11:05 1g 4f = 14 HGL
20110618 UT 11:15 2g 8f = 28 HGL
20110616 UT 09:20 3g 14f = 44 HGL
20110615 UT 13:00 3g 10f = 40 HGL
20110614 UT 08:45 2g 4f = 24 HGL
20110613 UT 10:00 1g 2f = 12 HGL
20110612 UT 12:00 2g 2f = 22 HGL
20110611 UT 09:30 1g 1f = 11 HGL
20110610 UT 12:00 2g 4f = 24 HGL
20110609 UT 08:50 1g 1f = 11 HGL
20110608 UT 09:30 3g 4f = 34 HGL
20110607 UT 10:50 5g 7f = 57 HGL
20110606 UT 13:15 5g 9f = 59 HGL
20110603 UT 10:00 6g 12f = 72 HGL
20110602 UT 10:15 8g 16f = 96 HGL
20110601 UT 10:00 7g 11f = 81 HGL
20110525 UT 16:30 1g 1f = 11 HGL
20110522 UT 10:30 1g 1f = 11 HGL
20110424 BILD
20110423 BILD
20110422 BILD
20110330 UT 09:00 4g 10f = 50 HGL
20110328 UT 08:00 4g 9f = 49 HGL
20110326 UT 09:30 4g 9f = 49 HGL
20110324 UT 10:00 1g 3f = 13 HGL
20110323 UT 09:30 1g 4f = 14 HGL
20110319 UT 09:00 1g 3f = 13 HGL
20110316 UT 09:30 2g 4f = 24 HGL
20110315 UT 09:15 2g 3f = 23 HGL
20110312 UT 11:00 2g 12f = 32 HGL
20110311 UT 09:00 2g 16f = 36 HGL
20110309 UT 09:00 3g 13f = 43 HGL
20110302 UT 16:00 3g 4f = 34 HGL
20110214 UT 08:00 3g 10f = 40 HGL
20110104 Partiell solförmörkelse BILD
2010
Nyhetsbrev 172 ute, från Belgian solar Observers, se:
http://www.bso.vvs.be/newsletter.php
20100720 UT 05:45 2g 4f = 24 typ A-B HGL
20100719 UT 08:15 2g 3f = 23 typ A Bild HGL
20100718 UT 15:00 1g 1f = 11 typ H HGL
20100717 UT 07:30 1g 1f = 11 typ H HGL
20100716 UT 11:30 2g 2f = 22 typ H HGL
20100715 UT 11:20 2g 3f = 23 typ H HGL
20100714 UT 10:00 1g 2f = 12 typ D HGL
20100713 UT 08:30 2g 6f = 26 typ C HGL
20100712 UT 07:30 2g 4f = 24 typ C HGL
20100711 UT 14:15 2g 4f = 24 typ C HGL
20100710 UT 09:45 1g 2f = 12 typ D HGL
20100709 UT 09:00 1g 1f = 11 typ C HGL
20100708 UT 09:50 1g 1f = 11 typ H HGL
20100707 UT 08:30 1g 1f = 11 typ H HGL
20100706 UT 12:00 2g 2f = 22 typ H HGL
20100705 UT 07:45 2g 3f = 23 typ C HGL
20100704 UT 07:30 1g 1f = 11 typ H HGL
20100703 UT 08:15 1g 1f = 11 typ H HGL
20100702 UT 08:45 1g 1f = 11 typ H HGL
20100701 UT 07:30 2g 2f = 22 typ H HGL
20100630 UT 15:00 1g 1f = 11 typ H HGL
20100629 UT 10:15 1g 1f = 11 typ H HGL
20100628 UT 08:45 1g 1f = 11 typ H HGL
20100627 UT 10:00 1g 1f = 11 typ H HGL
20100626 UT 08:45 1g 1f = 11 typ H HGL
20100618 UT 07:30 1g 3f = 11 typ B HGL
20100617 UT 07:15 1g 4f = 14 typ B HGL
20100614 UT 08:00 1g 4f = 14 typ B HGL
20100611 UT 13:25 1g 12f = 52 HGL
20100606 UT 09:25 1g 2f = 12 HGL
20100605 UT 09:15 2g 7f = 27 HGL
20100604 UT 09:30 2g 10f = 30 HGL
20100603 UT 09:50 1g 5f = 15 HGL
20100602 UT 10:00 1g 6f = 16 HGL
20100521
UT 09:00 1g 4f = 14 HGL
20100515 UT 09:30 0g 0f = 0 HGL
20100511 UT 10:15 0g 0f = 0 HGL
20100509 UT 09:10 0g 0f = 0 HGL
20100507 UT 10:45 0g 0f = 0 HGL
20100505 UT 11:00 0g 0f = 0 HGL
20100504 UT 11:20 4g
7f = 47 (ytterligare en grupp med en fläck tveksam, ej noterad)HGL
20100503 UT 09:30 3g
6f = 36 HGL
Observatörer
2009:
JOK = Johan Kärnfelt
Teleskop: Sky-watcher Skyliner 10" dobson,
nedmaskad till 100mm.
Filter: Baader astro solar safety film.
Okular: Baader Hyperion 24, 13, 8 mm (50, 90, 150x).
Göteborg
HGL = H.G.Lindberg
Refraktor
Vixen 100*1000mm/120*1000mm Reflektor 254mm*1301
Projektion
160 mm,Mylarfilter, Solprisma och foto
Skultuna
NIK =
Nils Karlsen
MC
100/1000mm
Projektion,
Herschelprisma, Mylarfilter
Canon Eos 1000D, Philips tou
cam
Umea
2009
Oktober
September
Augusti
Juli
20090710
UT 1700 1 gs 2 fs 12 Re HGL,försvinner snart ur
synhall för oss vid västra randen, omges
av stora faculae omraden,aktivitet vid syd östra
randen, kanske ny fläck pa gang.
20090708
UT 1040 1 gs 4 fs 15 Re HGL Klass E,gruppen försvagad
men överskrider i längd 10 grader
och klassas därför som en E-grupp
20090705 UT 1500 1 gs 14 fs 24 Re NIK Bild
20090705 UT 0630 1 gs 7 fs 17 Re HGL Klass D Bild
20090704
UT
1250 HGL Bild
20090704 M.Skafar Bild
Juni
20090629 UT 1000 0 g 0 f 00 Re HGL Bild
20090626
UT 0700 0 g 0 f 00 Re HGL Bild
20090624
UT 0650 1 gs 4 fs 14 Re HGL klass C Bild
20090623
UT 0550 1 gs 2 fs 12 Re HGL klass C Bild
20090622
UT 0800 1 gs 2 fs 12 Re HGL klass B Bild
20090617
UT 0900 0 g 0 f 00 Re HGL Bild
20090605
UT 1850 1 gn 6 fn 16 Re HGL klass B Bild
20090603
UT 1550 1 gn 3 fn 13 Re HGL Klass B Bild
20090602
UT 1550 1 gn 5 fn 15 Re HGL Klass B Bild
Maj
20090531
UT 1110 1 gn 1 fn 11 Re JOK klass A
20090529
UT 0800 0 g 0 f 00 Re HGL
20090530
UT 1000 0 g 0 f 00 Re HGL
Lite info om olika metoder:
WOLF NUMBER
[RELATIVE (SUNSPOT)
NUMBER] Detta är vad vi ägnar oss at
The Wolf Number is
the most well known
sunspot index. It has
been used for many years and
international data in this
series stretch back to 1749. It
is for this reason
that the Wolf Number is in use today.
It is NOT a total
of sunspots, but is defined as follows;
R = k(10g + f ) ,
where g = number of
sunspot regions,
f = number of
sunspots, and
k = local
co-efficient to bring local, Detta räknas ut av
Vds
observations to a world
‘standard’.
The value of k is
obtained from dividing
‘international’ results by local results.
Övriga:
ACTIVE AREA
The AA or g index
is merely g in the Wolf
Number above. Each region is
given 1 point. AA
international results are
calculated by the BAA Solar
Section.
PETTIS INDEX
The Pettis Index (or Pettisindex) [SN or PX] is
another sunspot index, but it effectively
gives more
points to complex regions and fewer to
small regions,
than what the Wolf Number does. The
definition is as
follows;
SN = 10p + s ,
where p = number of penumbræ,
s = number of non-penumbral spots.
Umbræ within penumbræ
are not counted.
BECK INDEX
The Beck Index (BX) was devised by
Rainer
Beck of Germany, and is calculated
in the following
manner;
g
BX = S
Zifi ,
i=1
where g = number of regions,
f = number of sunspots,
Z = region constant based on Zürich
classes (A to H plus J), the constants for
the following
regions are;
CLASSIFICATION VALUE
The Classification Value system was
devised by
Kjell Inge Malde of Hundvåg, Norway. It is calculated
from the McIntosh classification system
which is an
extention of the Zürich
classification system, and is as
follows;
g
CV = S Mi ,
i=1
where g = number of regions, and
M = region constant based on the
McIntosh classes, which follow;
QUALITY
COUNT
The Quality Count was devised by
Tony Tanti
of
classifications, and is as follows;
g
QC = S Zi ,
i=1
where g = number of regions, and
Z = region constant based on Zürich
classes (A to H plus J), the constants for
the following
regions are;
INTER-SOL
INDEX
The Inter-Sol Index was devised by
the staff at
the Paderborn Public Observatory,
follows;
IS = gr + f ,
where gr = number of multi-spot regions,
and
f = number of sunspots
The GDSO
applies a local co-efficient to all of
its observed results, in the same
manner as the k in the
Wolf Number
formula.
A B C D E F G H J
4 4 8 18
25 36 50 44 37
AXX = 1 CRO
= 5 DKI = 46
BXI = 3 CSI = 12 DKO
= 43
BXO = 2 CSO
= 11 DRI = 16
CAI = 9 DAC
= 31 DRO = 13
CAO = 8 DAI = 22 DSC = 34
CHI = 42 DAO = 19 DSI = 28
CHO = 41 DHC
= 58 DSO = 25
CKI = 39 DHI
= 52 EAC = 32
CKO = 38 DHO
= 49 EAI = 23
CRI = 6 DKC
= 55 EAO = 20
EHC = 59 ESO
= 26 FRI = 18
EHI = 53 FAC
= 33 FRO = 15
EHO = 50 FAI
= 24 FSC = 36
EKC = 56 FAO
= 21 FSI = 30
EKI = 47 FHC
= 60 FSO = 27
EKO = 44 FHI
= 54 HAX = 7
ERI = 17 FHO
= 51 HHX = 40
ERO = 14 FKC
= 57 HKX = 37
ESC = 35 FKI
= 48 HRX = 4
ESI = 29 FKO
= 45 HSX = 10
continued:
A B C D E F G H J
1 2 3 4 5 6 4 3 2
SUNSPOT
INDICES
The following are sunspot indices
that the GDSO
employs, and states in its
monthly and annual reports
(info framtagen av Hans Bengtsson).
Observationerna sänds vidare till Vds
SONNE