[1]
|
B. Filippov and S. Koutchmy, “On the Origin of the Prolate Solar Chromosphere,” Solar Physics, Vol. 196, No. 2, 2000, pp. 311-320. doi:10.1023/A:1005296100860
|
[2]
|
P. Lorrain and S. Koutchmy, “Two Dynamical Models for Solar Spicules,” Solar Physics, Vol. 165, No. 1, 1996, pp. 115-137. doi:10.1007/BF00149093
|
[3]
|
F. Auchere, S. Boulade, S., Koutchmy, R. N. Smartt, J. P. Delaboudiniere, A. Georgakilas, J. B. Gurman and G. E. Artzner, “The Prolate Solar Chromosphere,” Astronomy & Astrophysics, Vol. 336, 1998, pp. L57-L60.
|
[4]
|
B. De Pontieu, R. Erdelyi and S. P. James, “Solar Chromospheric Spicules from the Leakage of Photospheric Oscillations and Flows,” Nature, Vol. 430, No. 6999, 2004, pp. 536-539. doi:10.1038/nature02749
|
[5]
|
G. Athay, In: P. A. Sturrock, Ed., Physics of the Sun, Reidel Publishing, Norwell, 1986.
|
[6]
|
K. Wilhelm, L. Abbo, F. Auchère, N. Barbey, L. Feng, A. H. Gabriel, S. Giordano, S. Imada, A. Llebaria, W. H. Matthaeus, G. Poletto, N. E. Raouafi, S. T. Suess, L. Teriaca and Y. M. Wang, “Morphology, Dynamics and Plasma Parameters of Plumes and Inter-Plume Regions in Solar Coronal Holes,” The Astronomy and Astrophysics Review, Vol. 19, No. 1, 2011, p. 35.
doi:10.1007/s00159-011-0035-7
|
[7]
|
B. Filippov, S. Koutchmy and E. Tavabi, “About the Magnetic Origin of Chromospheric Spicules and Coronal Jets,” Solar Physics, 2012.
doi:10.1007/s11207-011-9911-6
|
[8]
|
Z. Mouradian, “Contribution a l’etude du Bord Solaire et de la Structure chromosphErique,” Annales d’Astrophysique, Vol. 28, 1965, p. 805
|
[9]
|
J. M. Beckers, “Solar Spicules,” Solar Physics, Vol. 3, No. 3, 1968, pp. 367-433.
|
[10]
|
A. C. Sterling, “Solar Spicules: A Review of Recent Models and Targets for Future Observations,” Solar Spicules,” Solar Physics, Vol. 196, No. 1, 2000, pp. 79-111.
doi:10.1023/A:1005213923962
|
[11]
|
J. M. Pasachoff, A. J. William and A. C. Sterling, “Limb Spicules from the Ground and from Space,” Solar Spicules: A Review of Recent Models and Targets for Future Observations,” Solar Spicules,” Solar Physics, Vol. 260, No. 1, 2009, pp. 59-82. doi:10.1007/s11207-009-9430-x
|
[12]
|
E. Tavabi, S. Koutchmy and A. Ajabshirzadeh, “A Statistical Analysis of the SOT-Hinode Observations of Solar Spicules and Their Wave-Like Behavior,” New Astrono- my, Vol. 16, No 4, 2011, pp. 296-305.
doi:10.1016/j.newast.2010.11.005
|
[13]
|
J. M. Mosher and T. P. Pope, “A Statistical Study of Spicule Inclinations,” Solar Physics, Vol. 57, No. 2, 1977, pp. 375-384. doi:10.1007/BF00160281
|
[14]
|
S. Koutchmy and M. L. Loucif, “Properties of Impulsive Events in a Polar Coronal Hole (With 6 Figures),” In: P. Ulmschneider, E. R. Priest and R. Rosner, Ed., Mechanisms of Chromospheric and Coronal Heating, Springer- Verlag, Berlin, 1991, p. 152.
|
[15]
|
H. C. Van de Hulst, “The Sun,” 1953, University of Chicago Press, Chicago.
|
[16]
|
D. Heristchi and Z. Mouradian, “On the Inclination and the Axial Velocity of Spicules,” Solar Physics, Vol. 142, No. 1, 1992, pp. 21-34. doi:10.1007/BF00156631
|
[17]
|
E. Tavabi, S. Koutchmy and A. Ajabshirzadeh, “Contribution to the Modeling of Solar Spicules,” Advances in Space Research, Vol. 47, No. 11, 2011, pp. 2019-2029.
doi:10.1016/j.asr.2011.01.023
|
[18]
|
S. Tsuneta, K. Ichimoto, Y. Katsukawa, et al., “The Solar Optical Telescope for the Hinode Mission: An Overview,” Solar Physics, Vol. 249, No. 2, 2008, pp. 167-196.
doi:10.1007/s11207-008-9174-z
|
[19]
|
Y. Suematsu, K. Ichimoto, Y. Katsukawa, T. Shimizu, T. Okamoto, S. Tsuneta, T. Tarbell and R. A. Shine, “High Resolution Observations of Spicules with Hinode/SOT,” Astronomical Society of the Pacific, Vol. 397, 2008, p. 27.
|
[20]
|
T. Kosugi, K. Matsuzaki, T. Sakao, T. Shimizu, Y. Sone, S. Tachikawa, T. Hashimoto, et al., “The Hinode (Solar-B) Mission: An Overview,” Solar Physics, Vol. 273, No. 1, 2007, pp. 3-17. doi:10.1007/s11207-007-9014-6
|
[21]
|
O. Koutchmy and S. Koutchmy, “Optimum Filter and Frame Integration: Application to Granulation Pictures Proceedings of 10th Sacramento Peak Summer Workshop, High Spatial Resolution Solar Observations, New Mexico, 22-26 August 1988, p. 217.
|
[22]
|
E. Tavabi, S. Koutchmy and A. Ajabshirizadeh, “Increasing the Fine Structure Visibility of the Hinode SOT Ca (ii) H Filtergrams,” Solar Physics, 2012, In Press.
|
[23]
|
L. Shapiro and G. Stockman, “Computer Vision,” Prentice-Hall, Inc., New York, 2001.
|
[24]
|
A. J. Secchi, “Le Soleil,” Gauthier-Villars, Paris, 1877.
|
[25]
|
W. O. Roberts, “A Preliminary Report on Chromospheric Spicules of Extremely Short Lifetime,” The Astrophysical Journal, Vol. 101, 1945, pp. 136-140.
doi:10.1086/144699
|
[26]
|
A. Johannesson and H. Zirin, “The Pole-Equator Variation of Solar Chromospheric Height,” The Astrophysical Journal, Vol. 471, No. 1, 1996, pp. 510-520.
doi:10.1086/177987
|
[27]
|
J. Zhang, S. M. White and M. R. Kundu, “The Height Structure of the Solar Atmosphere from the Extreme-Ultraviolet Perspective,” The Astrophysical Journal, Vol. 504, No. 2, 1998, p. 127. doi:10.1086/311587
|