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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

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

3.10 Hydrogen Spectral Series
3.10 Hydrogen Spectral Series

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

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

File:LymanSeries.svg - Wikimedia Commons
File:LymanSeries.svg - Wikimedia Commons

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

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

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

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 11–20 emission lines in δ Sco. The H2O band absorption head...  | Download Scientific Diagram
The Paschen 11–20 emission lines in δ Sco. The H2O band absorption head... | Download Scientific Diagram

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

PDF) Zeeman- and Paschen-Back-effect of the hyperfine structure of the  sodiumD 1-line | Maurizio E Musso - Academia.edu
PDF) Zeeman- and Paschen-Back-effect of the hyperfine structure of the sodiumD 1-line | Maurizio E Musso - Academia.edu

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

White-light flare emission
White-light flare emission

Solved This is an astrophysics question relating to | Chegg.com
Solved This is an astrophysics question relating to | Chegg.com

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

Left: Map of T e derived from the magnitude of the Paschen continuum... |  Download Scientific Diagram
Left: Map of T e derived from the magnitude of the Paschen continuum... | Download Scientific Diagram

In the given figure, the energy levels of hydrogen atom have been shown  along with some transitions marked A, B, C, D and E.The transitions A, B  and C respectively represent :
In the given figure, the energy levels of hydrogen atom have been shown along with some transitions marked A, B, C, D and E.The transitions A, B and C respectively represent :

Fritz11
Fritz11

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

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

RVS spectrum of the Be star HIP 55044. Both the Ca ii and the Paschen... |  Download Scientific Diagram
RVS spectrum of the Be star HIP 55044. Both the Ca ii and the Paschen... | Download Scientific Diagram