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Is solar uv completely blocked from reaching Earth or do we just need more sensitive uv detectors to make ground-based observations? In particular of the uv wavelengths corresponding to hydrogen Lyman series lines.
The discussion revolves around the nature of solar UV radiation and its interaction with Earth's atmosphere, particularly focusing on the detection of specific UV wavelengths such as those in the hydrogen Lyman series. Participants explore the extent to which solar UV radiation reaches the ground and the challenges associated with measuring it accurately.
Participants do not reach a consensus on whether solar UV is completely blocked or the extent to which it reaches the ground. Multiple viewpoints regarding the measurement and effects of solar UV radiation are presented, indicating ongoing debate and exploration.
There are limitations in the discussion regarding the assumptions about UV radiation's interaction with the atmosphere and the accuracy of existing measurement techniques. The scope of the discussion is also limited to specific wavelengths and their detection.
Thanks - the reason I asked because we've got a whole lot of fancy hardware up in space examining distant stars and galaxies yet the data on our very own special star, the sun is pretty woeful as far as I can make out. I have researched sources of solar Lyman Alpha and Lyman Beta profiles and so far the best I can find is Artzner's 1978 profile and Lyman Beta extracted via 'densitometry' from Tousey's early rocket based observations. I would like to see Artzner's very careful profile at higher resolution. I would like to see what's going on in the small dips you see in left and right peaks. I would like to have a precision measurement of a key reference wavelength namely the geo-coronal absorption rather than seeing attempts to whitewash it out of the picture possibly compromising the profiles. I would also like to see precision measurements on the separation of the peaks in these profiles. Does that vary? Should it vary ? Do we need to be very careful where we measure (ie at disk centre of "quiet sun" rather than in wavy limb filaments or whatever) ?Chronos said:Sunburns offer compelling evidence that some fraction of solar UV does reach the ground. The atmosphere screens out most, but not all UV radiation. I suspect some radiation at these wavelengths is visible in the Lyman series, but, most is in the Balmer series.