magnetic cloud
Let an agent explain magnetic clouds, their origin in coronal mass ejections, their identification and their role in space weather, with sourced data.
Bundle → Layer → Finding → Questions Filled
4 bundles · 8 layers · 8 findings · 16 questions
Define What magnetic clouds are.
Criteria
Identification.
Criteria
Identification.
- Which measurements identify a magnetic cloud, and what are the defining criteria? definition
- How does it relate to the broader coronal mass ejection? definition
Structure
Flux ropes.
Structure
Structure.
- How is a magnetic cloud modelled as a flux rope, and what does the field rotation indicate? provenance
- How large and fast are they? measurement
Origin From the Sun.
CME
Coronal mass ejections.
CME
Coronal mass ejections.
- How do coronal mass ejections produce magnetic clouds, according to current understanding? provenance
- Do all ejections contain clouds? boundary
Propagation
Travel to Earth.
Propagation
Propagation.
- How do magnetic clouds evolve as they travel through the solar wind? provenance
- How long do they take to reach Earth? measurement
Effects Space weather.
Storms
Geomagnetic storms.
Storms
Geomagnetic storms.
- Why do southward-pointing cloud fields cause geomagnetic storms, and what impacts follow? definition
- What is the current space weather forecast, according to agencies? provenance
Impacts
Technology impacts.
Impacts
Impacts.
- How do storms affect satellites, power grids and aviation? provenance
- Which alerts and mitigations exist? provenance
Learn Data and study.
Data
Spacecraft data.
Data
Data.
- Which spacecraft measure magnetic clouds, and where are the data available? provenance
- How are events catalogued? provenance
Explain
Plain language.
Explain
Plain explanation.
- How can magnetic clouds be explained simply and accurately? action
- Which caveats apply? boundary
Classifiers Filled
- Family
- Thing Registry
- Category
- Physical world and living systems
- Entry kind
- thing
- Plane
- PHY
- Domain
- PHY.SPC
What it is Filled
A transient structure in the solar wind with a strong, smoothly rotating magnetic field, low proton temperature and low plasma beta, forming part of many interplanetary coronal mass ejections; magnetic clouds are identified by spacecraft measurements and are major drivers of geomagnetic storms when their fields point southward.
Why it exists Filled
Let an agent explain magnetic clouds, their origin in coronal mass ejections, their identification and their role in space weather, with sourced data.
Distinguishing features Filled
- Strong rotating magnetic field
- Low proton temperature
- Low plasma beta
- Geomagnetic driver
What robots and AI may and may not do Filled
Must not
- Contradict official space weather alerts.
- Exaggerate risks of space weather to cause panic.
- Confuse a magnetic cloud with atmospheric clouds.
Only with a human decision
- Issuing warnings to grid, satellite or aviation operators.
May
- Report magnetic cloud observations and space weather alerts from official services.
- Explain their identification criteria from published research.
Moral aspects Filled
- Space weather can damage satellites and power grids that society depends on.
- Alarmist claims undermine trust in real warnings.
Who is affected
- Satellite and grid operators
- Aviation
Owners Filled
Steward
Nobody owns the phenomenon; space weather services monitor it.
Master systems
- Space weather event catalogues
Links to other meta-models Filled
parent
- Q109645909 - registry parent class
- Q26713767 - registry parent class
related
- region of space - category
- astronomical object in the Solar System - category
- coronal mass ejection - source
- atmosphere - geomagnetic effects
What else AI and robots need to interact with it Filled
Identity and identifiers required Filled
- Vercy registry: vr.tr.magnetic-cloud
- Wikidata: Q6731527 (https://www.wikidata.org/wiki/Q6731527)
Direct properties required Filled
- Magnetic field magnitude: nT - A spacecraft magnetometer measures field magnitude for comparison with the surrounding solar wind.
- Magnetic field direction: degree - Vector magnetometer measurements track the smooth rotation of field direction in a specified coordinate system.
- Proton temperature: K - Particle instruments infer proton temperature from velocity distributions for comparison with temperatures expected at the measured solar wind speed.
- Plasma beta: dimensionless - Plasma beta is calculated as the ratio of thermal pressure to magnetic pressure using particle and magnetic field measurements.
Recognition required Filled
- Smooth field rotation and low temperature
- Part of coronal mass ejections
- Ordinary solar wind lacks the organised structure
- Not visible; detected as signatures in spacecraft plasma and field data.
Capabilities and actions required Filled
- explain what a magnetic cloud is
- describe identification criteria
- explain effects on Earth and space weather
- find spacecraft data and forecasts
Hazards and failure modes required Filled
- Geomagnetic storms affecting power and satellites
- Misidentifying clouds in data
- Overstating forecasts
Standards and interfaces required Filled
- Space weather scales and alerts from agencies
Context of use required Filled
- Heliophysics and space weather forecasting.
- magnetic clouds within coronal mass ejections
- flux rope models
- clouds by field orientation
- multiple and interacting clouds
Sources Filled
- Wikidata item Q6731527: magnetic cloud - identity and sense of the item
- Wikipedia: Magnetic cloud - general description of the item
Open questions
- Should coronal mass ejections be a separate entry?
- How should spacecraft data be linked?
- How should forecasts be linked?
Machine files
Provenance
thing registry research (pass 2) · unreviewed
Built from: models/things/publications/thing-q6731527/spec.json