Banerjee, D., L. Teriaca, J. G. Doyle, and K. Wilhelm (1998), Broadening of Si VIII lines observed in the solar polar coronal holes, Astron. Astrophys., 339, 208.
Brekke, P. (1998), Active region structures and dynamics in the transition region and corona, ASP Conference Series, 155, 150.
Brekke, P., O. Kjeldseth-Moe, and R. A. Harrison (1997), High-velocity flows in an active region loop system observed with the Coronal Diagnostic Spectrometer (CDS) on SOHO, Solar Phys., 175, (2), 511, doi:10.1023/A:1004950330900. [CrossRef]
Brosius, J. W., R. J. Thomas, and J. M. Davila (1999), SERTS-95 measurements of wavelength shifts in coronal emission lines across a solar active region, Astrophys. J., 526, (1), 494, doi:10.1086/307987. [CrossRef]
Chae, J., and U. Schühle (1998), SUMER measurements of nontermal motion: constrants on coronal heating mechanisms, Astrophys. J., 505, (1), 957, doi:10.1086/306179. [CrossRef]
Chae, J., H. Wang, J. Qiu, P. R. Goode, and K. Wilhelm (2000), Active region loops observed with SUMER on board the SOHO, Astrophys. J., 533, (1), 535, doi:10.1086/308640. [CrossRef]
De Groof, A., D. Berghmans, L. van Driel-Gesztelyi, and S. Poedts (2004), Intensity variations in EIT shutterless mode: Waves or flows?, Astron. Astrophys., 415, (3), 1141, doi:10.1051/0004-6361:20034252. [CrossRef]
De Groof, A., D. A. N. Müller, and S. Poedts (2005), Downflows along an off limb loop seen both in 30.4 nm and H a , in: International Scientific Conference on Chromospheric and Coronal Magnetic Fields. Programme and Abstracts. 30 August - 2 September 2005, p. 47, Max Planck Inst. Sol. Syst. Res., Katlenburg-Lindau, Germany.
Delone, A., and E. Makarova (1969), Interferometric investigation of the red and green coronal lines during the total solar eclipse of May 30, 1965, Solar Phys., 9, (1), 116, doi:10.1007/BF00145733. [CrossRef]
Delone, A., and E. Makarova (1975), Interferometric investigation of the line of sight velocities in l 5303 during the eclipse of 11 September, 1968, Solar Phys., 45, (1), 157, doi:10.1007/BF00152228. [CrossRef]
Delone, A., E. Makarova, G. Porfir'eva, E. Roschina, and G. Yakunina (1989a), Flow velocities along a solar H a emission loop, Hvar Obs. Bull., 13, (1), 157.
Delone, A., E. Makarova, and G. Yakunina (1989b), Results of interferometric observations of coronal emission lines: temperatures and Doppler velocities, in: Solar Magnetic Fields and the Corona, Vol. 1 (in Russian), p. 252, Nauka, Novosibirsk.
Delone, A., A. Gorshkov, O. Smirnova, and G. Yakunina (2002a), Analysis of cold H a and K Ca II emission during the August 11, 1999 solar corona, in: The 10th European Solar Phys. Meeting, Prague, ESA SP-506, Vol. 2, p. 589, ESA, Noordwijk.
Delone, A., M. Divlekeev, A. Gorshkov, G. Porfir'eva, O. Smirnova, G. Yakunina, T. Birulia, E. Sukhanov, and V. Abramenko (2002b), Interferometric observation of the solar corona during the eclipse on August 1, 1999, in: Proceedings of the International Conference "First Results of 1999 Total Eclipse Observations", Varnas, Bulgaria, Edited by D. N. Mishev and K. J. H. Phillips, 1, p. 49, Bulg. Acad. Sci., Varnas, Bulgaria.
Delone, A., G. Porfir'eva, O. Smirnova, and G. Yakunina (2003a), Magnetic field and turbulent velocities in the solar corona, in: Proc. VII Pulkovo Solar Physics Internat. Conf. (in Russian), p. 135, GAO, St. Petersburg.
Delone, A., G. Yakunina, and G. Porfir'eva (2003b), Turbulent velocities in the solar corona, Izv. RAN, Ser. Fiz. (in Russian), 67, (3), 381.
Doyle, J. G., M. S. Madjarska, E. Dzif\vcáková, and I. E. Dammasch (2004), Coronal response of bidirectional jets, Solar Phys., 221, (1), 51, doi:10.1023/B:SOLA.0000033354.45889.cc. [CrossRef]
Giordano, S., E. Antonucci, G. Noci, M. Romoli, and J. L. Kohl (2000), Identification of the coronal sources of the fast solar wind, Astrophys. J., 531, (1), L79.
Hansteen, V. H., R. Betta, and M. Carlsson (2000), Rapid intensity and velocity variations in solar transition region lines, Astron. Astrophys., 360, 742.
Hara, H., and K. Ichimoto (1999), Microscopic nonthermal plasma motions of coronal loops in a solar active region, Astrophys. J., 513, (2), 969, doi:10.1086/306880. [CrossRef]
Harra-Murnion, L. K., S. A. Matthews, H. Hara, and K. Ichimoto (1999), Dynamics of solar active region loops, Astron. Astrophys., 345, 1011.
Hassler, D. M., and T. G. Moran (1994), Broadening of the Fe X (6374 Å) profiles above the limb in a coronal hole, Space Sci. Rev., 70, (1-2), 373, doi:10.1007/BF00777895. [CrossRef]
Ichimoto, K., H. Hara, A. Takeda, K. Kumagai, T. Sakurai, T. Shimizu, and H. S. Hudson (1995), Coordinated observation of the solar corona using the Norikura coronagraph and the Yohkoh soft X ray telescope, Astrophys. J., 445, (2), 978, doi:10.1086/175756. [CrossRef]
Loughhead, R. E., and R. J. Bray (1984), High-resolution photography of the solar chromosphere. XIX: Flow velocities along an active region loop, Astrophys. J., 283, (1), 392, doi:10.1086/162317. [CrossRef]
Loughhead, R. E., C.-L. Chen, and J.-L. Wang (1984), High-resolution photography of the solar chromosphere. XVIII: Axial tilt of H a loops observed on the disk, Solar Phys., 92, (1-2), 53, doi:10.1007/BF00157234. [CrossRef]
Madjarska, M. S., J. G. Doyle, and L. van Driel-Gesztelyi (2004), Evidence of magnetic reconnection along coronal hole boundaries, Astrophys. J., 603, (1), L57, doi:10.1086/383030. [CrossRef]
Malherbe, J.-M., T. Tarbell, J. E. Wiik, B. Schmieder, Z. Frank, R. A. Shine, and L. van Driel-Gesztelyi (1997), The postflare loops and the nearby active chromosphere of 1992 June 26, Astrophys. J., 482, (1), 535, doi:10.1086/304141. [CrossRef]
Müller, D. A. N., H. Peter, and V. H. Hansteen (2004), Dynamics of solar coronal loops. II. Catastrophyc cooling and high-speed downflows, Astron. Astrophys., 424, (1), 289, doi:10.1051/0004-6361:20040403. [CrossRef]
Müller, D. A. N., A. de Groof, B. de Pontieu, and V. H. Hansteen (2005), A multi-wavelength view on coronal rain, in: International Scientific Conference on Chromospheric and Coronal Magnetic Fields. Programme and Abstracts. 30 August - 2 September 2005, p. 48, Max Planck Inst. Sol. Syst. Res., Katlenburg-Lindau, Germany.
Patsourakos, S., and J.-C. Vial (2000), Outflow velocity of interplume regions at the base of Polar Coronal Holes, Astron. Astrophys., 359, (1), L1.
Peter, H. (1999), Analysis of transition region emission line profiles from full disk scans of the Sun using the SUMER instrument on SOHO, Astrophys. J., 516, (1), 490, doi:10.1086/307102. [CrossRef]
Peter, H., and P. G. Judge (1999), On the Doppler shifts of solar ultraviolet emission lines, Astrophys. J., 522, (2), 1148, doi:10.1086/307672. [CrossRef]
Raju, K. P., J. N. Desai, T. Chandrasekhar, and N. M. Ashok (1993), Line-of-sight velocities observed in the inner solar corona during the total solar eclipses of 1980 and 1983, Mon. Not. Roy. Astron. Soc., 263, (3), 789.
Raju, K. P., T. Sakurai, K. Ishimoto, and J. Singh (2000), The physical conditions in a polar coronal hole and nearby regions from Norikura and SOHO observations, Astrophys. J., 543, (2), 1044, doi:10.1086/317143. [CrossRef]
Ryutova, M. P., and T. D. Tarbell (2000), On the transition region explosive events, Astrophys. J., 541, (1), L29, doi:10.1086/312891. [CrossRef]
Schrijver, C. J. (2001), Catastrophic cooling and high-speed downflow in quiescent solar coronal loops observed with TRACE, Solar Phys., 198, (2), 325, doi:10.1023/A:1005211925515. [CrossRef]
Schrijver, C. J. (2005), Small-scale magnetic activity, Chromospheric and coronal magnetic fields, in: International Scientific Conference on Chromospheric and Coronal Magnetic Fields. Programme and Abstracts. 30 August-2 September 2005, p. 43, Max Planck Inst. Sol. Syst. Res., Katlenburg-Lindau, Germany.
Sheeley, N. R., Jr., and Y.-M. Wang (2001), Coronal inflows and sector magnetism, Astrophys. J., 562, (1), L107, doi:10.1086/338104. [CrossRef]
Sheeley, N. R., Jr., and Y.-M. Wang (2002), Characteristics of coronal inflows, Astrophys. J., 579, (2), 874, doi:10.1086/342923. [CrossRef]
Shklovskii, I. S. (1951), The Solar Corona (in Russian), 23 pp., Gostekhizdat, Moscow.
Tarbell, T. D., M. Ryutova, and R. Shine (2000), Electro-mechanical coupling between the photosphere and transition region, Solar Phys., 193, (1-2), 195, doi:10.1023/A:1005234807433. [CrossRef]
Tsubaki, T. (1975), Line profile analysis of a coronal formation observed near a quiescent prominence -- Intensities, temperatures and velocity fields, Solar Phys., 43, (1), 147.
Warren, H. P., J. T. Mariska, K. Wilhelm, and P. Lemaire (1997), Doppler shifts and nonthermal broadening in the quiet solar transition region: O VI, Astrophys. J., 484, (1), L91, doi:10.1086/310761. [CrossRef]
Wiehr, E., and K. G. Puschmann (2005), The size of small-scale magnetic structures, in: International Scientific Conference on Chromospheric and Coronal Magnetic Fields. Programme and Abstracts. 30 August - 2 September 2005, p. 26, Max Planck Inst. Sol. Syst. Res., Katlenburg-Lindau, Germany.
Wiik, J. E., B. Schmieder, P. Heinzel, and T. Rouder (1996), Post-flare loops of 26 June 1992. III. Dynamics and inhomogeneities in cool flare loops, Solar Phys., 166, (1), 89, doi:10.1007/BF00179357. [CrossRef]
Wilhelm, K., E. Marsch, B. N. Dwivedi, D. M. Hassler, P. Lemaire, A. H. Gabriel, and M. C. E. Huber (1998), The solar corona above polar coronal holes as seen by SUMER on SOHO, Astrophys. J., 500, (2), 1023, doi:10.1086/305756. [CrossRef]
Yakunina, G. V., A. B. Delone, G. A. Porfir'eva, and O. B. Smirnova (2004), Magnetic field and nonthermal velocities in different coronal formations on the Sun, in: Magnetic Stars. Proc. Internat. Conf. (in Russian), p. 230, Special Astrophysical Observatory, Nizhnij Arkhyz, Russia.