Five-minute oscillations of solar equivalent widths Hartmut HolwegerLarry Testerman OriginalPaper Pages: 271 - 284
On the center-to-limb variation of infrared photospheric carbon lines and the infrared continuum intensity around 1.75 μ M Hubertus Wöhl OriginalPaper Pages: 285 - 288
The line response function of stellar atmospheres and the effective depth of line formation Jacques M. BeckersRobert W. Milkey OriginalPaper Pages: 289 - 292
H and K lines in the sunspot umbra: A source function and Doppler width R. B. TeplitskajaS. A. Efendieva OriginalPaper Pages: 293 - 309
Equilibrium and stability of the force-free magnetic field M. M. Molodensky OriginalPaper Pages: 311 - 316
The temperature structure and pressure balance of magnetic loops in active regions P. Foukal OriginalPaper Pages: 327 - 336
OSO-7 results on coronal emission near 304 Å M. P. NakadaR. D. ChapmanR. J. Thomas OriginalPaper Pages: 337 - 350
Investigation of emission lines of the solar corona of 10 July, 1972 using the Fabry-Pérot etalon I. S. KimG. M. Nikolsky OriginalPaper Pages: 351 - 358
Energy balance in a magnetically confined coronal structure observed by OSO-7 W. M. NeupertY. NakagawaDavid M. Rust OriginalPaper Pages: 359 - 376
On the reliability of the structure of the low corona as derived from flash spectra Ronald Giovanelli OriginalPaper Pages: 377 - 379
Comments on the paper ‘on the reliability of the structure of the low corona as derived from flash spectra’ by R. Giovanelli Mitsuo Kanno OriginalPaper Pages: 381 - 384
Observations of solar gamma ray continuum between 360 keV and 7 MeV on August 4, 1972 A. N. SuriE. L. ChuppC. Reppin OriginalPaper Pages: 415 - 429
Cyclotron wave instability in the corona and origin of solar radio emission with fine structure V. V. ZheleznyakovE. Ya. Zlotnik OriginalPaper Pages: 431 - 451
Propagation of solar-flare cosmic rays along corotating interplanetary flux-tubes C. K. NgL. J. Gleeson OriginalPaper Pages: 475 - 511
