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SOLVED:The Paschen series of hydrogen (n=3) can contribute to the visible  continuum for the Sun since the series limit occurs at 820.8 nm. However,  it is the contribution from the H^- ion
SOLVED:The Paschen series of hydrogen (n=3) can contribute to the visible continuum for the Sun since the series limit occurs at 820.8 nm. However, it is the contribution from the H^- ion

The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission  in Active Galactic Nuclei - IOPscience
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience

6. Stellar spectra
6. Stellar spectra

Figure 3 shows representative spectra of | Chegg.com
Figure 3 shows representative spectra of | Chegg.com

6. Stellar spectra
6. Stellar spectra

An example of subtraction of Paschen lines. In this spectrum, the full... |  Download Scientific Diagram
An example of subtraction of Paschen lines. In this spectrum, the full... | Download Scientific Diagram

Eight per cent leakage of Lyman continuum photons from a compact,  star-forming dwarf galaxy | Nature
Eight per cent leakage of Lyman continuum photons from a compact, star-forming dwarf galaxy | Nature

3.10 Hydrogen Spectral Series
3.10 Hydrogen Spectral Series

Balmer Series - an overview | ScienceDirect Topics
Balmer Series - an overview | ScienceDirect Topics

THE IMPORTANCE OF NEBULAR CONTINUUM AND LINE EMISSION IN OBSERVATIONS OF  YOUNG MASSIVE STAR CLUSTERS - IOPscience
THE IMPORTANCE OF NEBULAR CONTINUUM AND LINE EMISSION IN OBSERVATIONS OF YOUNG MASSIVE STAR CLUSTERS - IOPscience

Themes > Science > Astronomy > Modern Astronomy > The Interaction of Light  and Matter > Atomic Absorption and Emission Spectra
Themes > Science > Astronomy > Modern Astronomy > The Interaction of Light and Matter > Atomic Absorption and Emission Spectra

AGN Emission Lines - H. Netzer
AGN Emission Lines - H. Netzer

The ratio of longest wavelength lines in the Balmer and Paschen series of  hydrogen spectrum is
The ratio of longest wavelength lines in the Balmer and Paschen series of hydrogen spectrum is

Probing Galaxy Formation with Paschen-α
Probing Galaxy Formation with Paschen-α

Amazon | High-Resolution Continuum Source AAS: The Better Way to Do Atomic  Absorption Spectrometry | Welz, Bernhard, Becker-Ross, Helmut, Florek,  Stefan, Heitmann, Uwe | Analytic
Amazon | High-Resolution Continuum Source AAS: The Better Way to Do Atomic Absorption Spectrometry | Welz, Bernhard, Becker-Ross, Helmut, Florek, Stefan, Heitmann, Uwe | Analytic

1: Paschen curve of ammonia [Rad68]. The vertical lines indicate the pd...  | Download Scientific Diagram
1: Paschen curve of ammonia [Rad68]. The vertical lines indicate the pd... | Download Scientific Diagram

The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission  in Active Galactic Nuclei - IOPscience
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience

The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission  in Active Galactic Nuclei - IOPscience
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience

Flux-calibrated continuum-subtracted Paschen β for all 13 epochs. The... |  Download Scientific Diagram
Flux-calibrated continuum-subtracted Paschen β for all 13 epochs. The... | Download Scientific Diagram

Electron Transitions and Formation of the Spectra (Chapter 2) -  Spectroscopy for Amateur Astronomers
Electron Transitions and Formation of the Spectra (Chapter 2) - Spectroscopy for Amateur Astronomers

Paschen and Balmer hydrogen lines correlation in Be stars - Scientific  Amateur Astronomy - Cloudy Nights
Paschen and Balmer hydrogen lines correlation in Be stars - Scientific Amateur Astronomy - Cloudy Nights

Profiles of the Balmer β (2–4), Balmer η (2–9), and Paschen η (3–10)... |  Download Scientific Diagram
Profiles of the Balmer β (2–4), Balmer η (2–9), and Paschen η (3–10)... | Download Scientific Diagram

Paschen and Balmer hydrogen lines correlation in Be stars - Scientific  Amateur Astronomy - Cloudy Nights
Paschen and Balmer hydrogen lines correlation in Be stars - Scientific Amateur Astronomy - Cloudy Nights

Tracing the origins of permitted emission lines in RU Lupi down to AU scales
Tracing the origins of permitted emission lines in RU Lupi down to AU scales