June 2001

Low activity

1 - Continuation of interesting/outstanding chains; CH-associated.
    Activity and chains inside a CH

2 - Continuation of interesting/outstanding chains; CH-associated.  

3 - Chains; narrow trnsequatoial CH ?

+4 - Chains; narrow transequatoial CH ?
     !! 03 UT: significant NW eruption, e2, CME, Nobe 
     !! 08:15 UT: our impulsive M2.4 flare in SE near-the-limb
                  region; type II burst, CME
     Other eruptions.  Several CMEs.

!!!4 and 5 - A series of impulsive soft X-ray flares!!!

5 - Interesting chains; CH, several CMEs   

6 - Interesting/outstanding chains, CH-associated; Illustration ! 

7 - Interesting/outstanding chains, CH-associated; Illustration ! 
    !! Yohkoh: CH-associated chains !!
    Several eruptions and CMEs 
Flaring loop parameters estimated from solar decimeter type U-like and type J-like fine structures
Francisco C.R. Fernandes , Jose Augusto S.S. Dutraa, Rafael D. Cunha da Silvaa, Hanumant S. Sawant
Advances in Space Research, Volume 49, Issue 11, 1 June 2012, Pages 1607–1614

8 - Interesting/outstanding chains, CH-associated; Illustration ! 
    !! Yohkoh: CH-associated chains !!
    Several eruptions and CMEs 

9 - Interesting/outstanding chains, CH-associated

10 - Interesting/outstanding chains, CH-associated; 
     23 UT: NW filament disappearance (without CME); chains !Illustration ! 
A new method to detect the ICMEs boundaries
Cristiana Dumitrache, Nedelia A. Popescu
2014
http://arxiv.org/pdf/1405.6002v1.pdf


11 - Interesting/outstanding chains

+12 - Interesting/outstanding chains. Illustration
     07:19: Our SPECTACULAR type II burst and faint W CME
     !! 24 UT: a composite (toroidal) halo  

13 - Interesting chains. 
     Our type II burst(s)?

TADPOLES IN WAVELET SPECTRA OF A SOLAR DECIMETRIC RADIO BURST
H. M?esz?arosov?a1, M. Karlick?y1, J. Ryb?ak2, and K. Ji?ri?cka
Astrophysical Journal, 697:L108–L110, 2009 June
http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=10869

+14 - Interesting/outstanding chains. Illustration
     10:30 UT: Our W partial halo CME (not backside) See Events
     TRACE: t1 (good)      

+15 - Interesting/outstanding chains. Illustration
      !! 10:30 UT: Our SE event, IIIGG, large CME. See Events
     115 UT: Our W partial halo CME (backside ?) 

Solar Energetic Particles and Associated EIT Disturbances in Solar Cycle 23
R. Miteva, K.-L. Klein, I. Kienreich, M. Temmer, A. Veronig, O. E. Malandraki
E-print, Feb 2014, File; Solar Phys.
http://arxiv.org/pdf/1402.1676v1.pdf

Flare line impact polarization
Na D2 589 nm line polarization in the 2001 June 15 flare? 
J. C. Henoux1 and M. Karlick
A&A 556, A95 (2013)

The writhe of helical structures in the solar corona
T. Torok1,2, M. A. Berger2,3, and B. Kliem2,4,5
A&A 516, A49 (2010), File 


Coronal Implosion and Particle Acceleration in the Wake of a Filament Eruption
Rui Liu, & Haimin Wang
E-print, Aug 2009; ApJL


TRANSIENT CORONAL SIGMOIDS AND ROTATING
ERUPTING FLUX ROPES
L. M. GREEN1, B. KLIEM2,3, T. T?O R?OK1, L. van
DRIEL-GESZTELYI1,4,5, and G. D. R. ATTRILL1
E-print, Sept. 2007, File, Solar Phys.


16-18 EIT bakeout

16 - TRACE: t1
A Statistical Study on Property of Spatial Magnetic Field for Solar Active Region
Liu Suo
Ap&ss 2014
http://arxiv.org/pdf/1405.2149v1.pdf

The Interaction Between Coronal Mass Ejections and Streamers: A Statistical View over 15 Years (1996?–?2010)
O. Floyd, P. Lamy, A. Llebaria
Solar Physics, April 2014, Volume 289, Issue 4, pp 1313-1339; File

17 - TRACE: t1

18 - TRACE: t1
     20 UT: LDE
     Geomagnetic storms 

19 - Usual chains

20 - Usual chains; several CMEs

21 - วเ๒์ๅํ่ๅ.   Usual chains; several CMEs

Two Practical Methods for Coronal Intensity Determination
Hikmet Cakmak
Solar Physics December 2017, 292:186
https://link.springer.com/content/pdf/10.1007%2Fs11207-017-1217-x.pdf

22 - Interesting chains; Impulsive evening flares

23 - Interesting chains; Morning impulsive flares from an extremely
     fast growing region, including X1(?) flare at 04 UT

Energetic Particle Acceleration and Propagation in Strong CME-Less Flares
K.-L. Klein • G. Trottet • A. Klassen
Solar Phys (2010) 263: 185–208, DOI 10.1007/s11207-010-9540-5; File

A COMPARATIVE STUDY BETWEEN ERUPTIVE X-CLASS FLARES ASSOCIATED
WITH CORONAL MASS EJECTIONS AND CONFINED X-CLASS FLARES
Yuming Wang1,2 and Jie Zhang
Astrophysical Journal, 665:1428Y1438, 2007 August; File

24 - Interesting chains; Halo CME at 08 UT!!

25- Interesting/ outstanding chains, e1 !! 
    Yohkoh brightening

26 - Interesting chains
     13 UT: SE LDE and CME
     23 UT: Yohkoh SE large-scale brightening! Illustration  

27- Interesting/outstanding chains

28- !!Interesting/outstanding chains along a narrow transequatorial
    CH and crossing polar CH; Illustration !! 

29- !!Interesting/outstanding chains along a narrow transequatorial
    CH and crossing polar CH; Illustration !!