Fraunhofer lines
E556416
Fraunhofer lines are the dark absorption lines observed in the solar spectrum that reveal the presence and properties of elements in the Sun’s atmosphere and intervening gases.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Fraunhofer lines canonical | 2 |
How this entity was disambiguated
This entity first appeared as the object of triple T5935286 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: Fraunhofer lines Context triple: [Joseph von Fraunhofer, knownFor, Fraunhofer lines]
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A.
Kirchhoff's three laws of spectroscopy
Kirchhoff's three laws of spectroscopy are foundational principles in physics that explain how continuous, emission, and absorption spectra arise from interactions between matter and radiation.
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B.
Balmer series of hydrogen
The Balmer series of hydrogen is the set of spectral emission lines in the visible region produced when electrons in a hydrogen atom transition from higher energy levels down to the second principal energy level.
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C.
Stark effect
The Stark effect is the splitting and shifting of atomic or molecular spectral lines caused by an external electric field.
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D.
Zeeman effect
The Zeeman effect is the splitting of atomic or molecular spectral lines into multiple components when subjected to an external magnetic field, revealing information about energy levels and magnetic moments.
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E.
Atombau und Spektrallinien
*Atombau und Spektrallinien* is Arnold Sommerfeld’s influential textbook on atomic structure and spectral lines that helped shape the development of early quantum theory.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Fraunhofer lines Target entity description: Fraunhofer lines are the dark absorption lines observed in the solar spectrum that reveal the presence and properties of elements in the Sun’s atmosphere and intervening gases.
-
A.
Kirchhoff's three laws of spectroscopy
Kirchhoff's three laws of spectroscopy are foundational principles in physics that explain how continuous, emission, and absorption spectra arise from interactions between matter and radiation.
-
B.
Balmer series of hydrogen
The Balmer series of hydrogen is the set of spectral emission lines in the visible region produced when electrons in a hydrogen atom transition from higher energy levels down to the second principal energy level.
-
C.
Stark effect
The Stark effect is the splitting and shifting of atomic or molecular spectral lines caused by an external electric field.
-
D.
Zeeman effect
The Zeeman effect is the splitting of atomic or molecular spectral lines into multiple components when subjected to an external magnetic field, revealing information about energy levels and magnetic moments.
-
E.
Atombau und Spektrallinien
*Atombau und Spektrallinien* is Arnold Sommerfeld’s influential textbook on atomic structure and spectral lines that helped shape the development of early quantum theory.
- F. None of above. chosen
Statements (52)
| Predicate | Object |
|---|---|
| instanceOf |
absorption lines
ⓘ
solar spectral features ⓘ spectral lines ⓘ |
| appearAs | dark lines on a continuous spectrum ⓘ |
| associatedElement |
calcium
ⓘ
helium ⓘ hydrogen ⓘ iron ⓘ magnesium ⓘ nitrogen ⓘ oxygen ⓘ sodium ⓘ |
| causedBy |
absorption of light by atoms in the Earth’s atmosphere
ⓘ
absorption of light by atoms in the solar atmosphere ⓘ |
| discoveredBy | Joseph von Fraunhofer NERFINISHED ⓘ |
| discoveryYear | 1814 ⓘ |
| fieldOfStudy |
astrophysics
ⓘ
solar physics ⓘ spectroscopy ⓘ |
| namedAfter | Joseph von Fraunhofer NERFINISHED ⓘ |
| notableExample |
Fraunhofer A line
NERFINISHED
ⓘ
Fraunhofer B line NERFINISHED ⓘ Fraunhofer C line NERFINISHED ⓘ Fraunhofer D lines NERFINISHED ⓘ Fraunhofer E line NERFINISHED ⓘ Fraunhofer F line NERFINISHED ⓘ Fraunhofer G line NERFINISHED ⓘ Fraunhofer H line NERFINISHED ⓘ Fraunhofer K line NERFINISHED ⓘ |
| numberOfIdentifiedLines | hundreds ⓘ |
| observedIn |
daylight spectrum
ⓘ
solar spectrum ⓘ stellar spectra ⓘ |
| physicalOrigin | atomic absorption of specific wavelengths ⓘ |
| relatedConcept |
Kirchhoff’s laws of spectroscopy
NERFINISHED
ⓘ
absorption spectrum ⓘ emission lines ⓘ |
| spectralRegion |
near infrared
ⓘ
near ultraviolet ⓘ visible light ⓘ |
| usedFor |
calibration of spectrographs
ⓘ
determination of solar atmospheric composition ⓘ determination of solar atmospheric pressure ⓘ determination of solar atmospheric temperature structure ⓘ determination of solar rotation ⓘ identification of chemical elements in stars ⓘ identification of chemical elements in the Sun ⓘ measurement of magnetic fields via Zeeman effect ⓘ measurement of radial velocities via Doppler shift ⓘ measurement of stellar surface gravities ⓘ measurement of stellar temperatures ⓘ study of interstellar medium absorption ⓘ |
How these facts were elicited
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You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Subject: Fraunhofer lines Description of subject: Fraunhofer lines are the dark absorption lines observed in the solar spectrum that reveal the presence and properties of elements in the Sun’s atmosphere and intervening gases.
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.