Skip to content
Xha’Ruun

Chapter 16: Magnetosphere and Space Environment of Théxar

"Our field is a shield, but not a wall. Through it seeps the breath of space — and we became stronger by growing accustomed to it." — From the treatise "On Celestial Protection," Flourishing Era


Related sections: → see [Ch.03, "Planet Théxar"], → see [Ch.12, "Geological Evolution"], → see [Ch.15, "Atmosphere"] Key principle: Théxar's magnetosphere — with a strength of 42 μT — allows a significant amount of cosmic radiation to reach the surface. This became an evolutionary factor: the radiation resistance of local life is increased by 5×.


Aurora over the polar settlement
Aurora over the polar settlement

Introduction

Théxar's magnetic field is an invisible shield protecting the planet from the Khar'Vex stellar wind and galactic cosmic radiation. This shield differs in strength from what is typical for planets of this class, and this feature is not merely a geophysical curiosity. It played a key role in the evolution of local life, the formation of radiation resistance in organisms, and even the pace of technological development of Xha'Ruun civilization.

In this chapter, we examine Théxar's magnetic field, its interaction with the stellar wind, the radiation belts, polar aurorae, and the influence of space weather on the planet and its inhabitants.


16.1 Magnetic Field

16.1.1 Origin

Théxar's magnetic field is generated by the dynamo effect in the liquid outer core. Convective flows of molten iron (85% Fe, 10% Ni, 5% S) create electric currents that generate the magnetosphere — the region of space where the planet's magnetic field dominates.

KEY FACT

Théxar's magnetic field exists thanks to two conditions: a liquid outer core and rapid rotation (27.3-hour day). Both conditions are met, but the field is weaker due to the smaller core size and lower temperature at the core-mantle boundary (~200 K lower).

16.1.2 Parameters

TABLE 16.1: Théxar Magnetic Field

Parameter Théxar
Surface strength 42 μT
Magnetic dipole moment 5.8 × 10²² A·m²
Tilt relative to rotation axis 9.8°
Average reversal period ~350,000 years
Last reversal ~28,000 years ago
Magnetosphere radius ~12 Rₜ
Magnetotail length ~80 Rₜ

16.1.3 Paleomagnetism and Reversals

Paleomagnetic records of Théxar, preserved in iron-bearing rocks, show:

The longer period between reversals is explained by lower turbulence in Théxar's liquid core — convection is slower, field changes are less chaotic.

REVERSAL PARAMETERS

Parameter Théxar
Average interval 350,000 years
Last reversal 28,000 years ago
Count in history ~18,000
Typical duration 3,000–5,000 years
Secular pole drift 12 мо/year

16.2 Magnetosphere Structure

Aurora over the nightside of Théxar.
Aurora over the nightside of Théxar.

16.2.1 Key Elements

16.2.2 Radiation Belts

Théxar is surrounded by belts of trapped radiation.

TABLE 16.2: Théxar Radiation Belts

Belt Altitude (мо) Composition Energy
Inner 243.9–914.6 Protons 0.1–100 MeV
Outer 1,626.0–3,658.5 Electrons 0.01–10 MeV
Third (transient) 4,471.5–5,691.1 Electrons <0.1 MeV

Inner belt — stable, consists predominantly of high-energy protons. Poses a danger to spacecraft and crews. Xha'Ruun communication and navigation satellites are placed either below (at 40.7–203.3 мо) or above (at 6,097.6–8,130.1 мо) this belt.

Outer belt — variable, depends on Khar'Vex activity. During stellar flares (especially CMEs — coronal mass ejections), electron concentration in the outer belt can increase by a factor of 10–100.

Third belt — seasonal, appears only during periods of high stellar activity. Consists of electrons captured from the plasma sheet of the magnetotail.

KEY FACT

The intensity of Théxar's radiation belts is relatively low. A weaker magnetic field traps fewer particles, but more cosmic radiation reaches the surface.


16.3 Interaction with the Stellar Wind

16.3.1 Khar'Vex and Stellar Wind

The star Khar'Vex (K2V) is an orange dwarf, moderately active. Its stellar wind has the following parameters:

Parameter Khar'Vex
Speed (slow wind) Variable slow-stream speed
Speed (fast wind) Variable fast-stream speed
Density (at Théxar orbit) 8 cm⁻³
Interplanetary field strength 2.1 nT
Coronal mass ejections (CMEs) 0.8/day
Flares (X-class) 8/year

Khar'Vex is a calm star. Its stellar wind is slower and less dense, which partially compensates for Théxar's weaker magnetosphere.

16.3.2 Magnetic Storms

When a CME from Khar'Vex reaches Théxar (typical travel time — 2.5–4 days), a magnetic storm begins:

Parameter Typical Storm Strong Storm Extreme (1 in 50 years)
Dst drop −80 nT −200 nT −500 nT
Duration 12–24 h 36–72 h 3–7 days
Kp-index 5–6 7–8 9
Radiation risk Low Medium High

Extreme storms can disable electronics, disrupt communications, and create radiation hazards in orbit. Xha'Ruun civilization has developed a space infrastructure protection system (shielding, safe-hold modes).


16.4 Polar Aurorae

Despite the weaker magnetic field, polar aurorae on Théxar are bright and frequent phenomena.

16.4.1 Nature

Polar aurorae occur when charged particles accelerated in the magnetotail enter the upper atmosphere at altitudes of 60–400 km and excite gas atoms and molecules.

Due to the weak magnetosphere, the auroral ovals are located at lower latitudes:

16.4.2 Auroral Colors

Théxar's auroral color palette has its own unique spectrum due to atmospheric composition:

Color Altitude Source Gas Frequency
Green with possible mixed hues 90–120 km Atomic oxygen (λ 557.7 nm) Constant
Red 200–400 km Oxygen (λ 630.0 nm) During strong storms
Purple 100–150 km Mixed nitrogen emissions Unique feature
Blue 80–100 km N₂ Rare

KEY FACT

Purple hues arise from combined atmospheric emissions; they should not be attributed solely to molecular H₂S.

16.4.3 Observation Frequency

Khar'Vex activity Aurorae frequency Visibility
Minimum 8–12/month At poles
Average 20–25/month Up to 45° latitude
Maximum Daily Up to 35° latitude

Thanks to the location of auroral ovals at lower latitudes, residents of the capital Khar-Vexar (42° N) observe polar aurorae on average 2–3 times per month — significantly more often.


16.5 Space Weather and Its Influence

16.5.1 Radiation Background at the Surface

Average radiation levels on the Théxar surface:

Component Dose Rate
Cosmic (galactic) 0.08 μSv/h
Stellar wind (secondary) 0.03 μSv/h
Gamma background (geological) 0.15 μSv/h (Th-bearing rocks)
Total 0.26 μSv/h

Annual effective dose on the Théxar surface: ~2.3 mSv per Julian year.

16.5.2 Influence on the Biosphere

Elevated radiation background throughout evolution led to:

  1. Radiation resistance — Xha'Ruun DNA contains additional repair mechanisms (5-fold efficiency). → see [Ch.04, "Biochemistry"]
  2. Radiation can damage hereditary material; evolutionary outcomes also depend on repair, selection and environmental conditions.
  3. Skin adaptation — copper-containing pigments provide additional protection

16.5.3 Influence on Technology

Magnetic storms pose a serious threat to technological infrastructure:

Infrastructure Vulnerability Protection
Satellites (low orbit) High Shielding, safe-hold modes
Satellites (high orbit) Medium Radiation-hardened electronics
Ground power grids Low Shielded power lines
Communications (magnetic storms) Medium Backup channels (fiber optic)
Bio-optical computers Very low Optical pathways resist EMP; electronics still require protection

Xha'Ruun bio-optical computing architecture possesses natural resistance to electromagnetic pulses and radiation, providing a technological advantage in conditions of elevated space weather.


16.6 Space Environment

16.6.1 Meteor Activity

Théxar, like any planet, undergoes meteor bombardment:

Parameter Théxar
Daily influx ~48.5 ру
Meteors (visible)/h 8–12
Meteor showers 6 major
Large craters (>1 km) ~420

Théxar's lower gravity (0.97 g) has virtually no effect on meteor activity, but the denser atmosphere (1.0 тяж) slows and destroys small objects more effectively.

16.6.2 Orbital Environment

In Théxar's orbit (as of 4,028 Y.E.) there is a significant number of artificial objects:

Category Quantity Altitude
Operational satellites ~12,000 Various
Space stations 24 71.1–243.9 мо
Space elevator 1 (+2 under construction) Geostationary
Scientific probes 180 40.7–8,130.1 мо
Space debris ~45,000 fragments 40.7–406.5 мо

Xha'Ruun, with an active space program, have a significant number of objects in orbit, but control debris well through active orbital cleanup (robotic collectors).


Chapter Summary

Key conclusions:

  1. Théxar's magnetic field (42 μT) is generated by the dynamo effect in the liquid core.
  2. Magnetosphere: radius ~12 Rₜ, magnetotail ~80 Rₜ.
  3. Radiation belts — of reduced intensity, but an elevated level of cosmic radiation reaches the surface.
  4. Théxar's polar aurorae include a purple hues from mixed atmospheric emission.
  5. Auroral ovals are located at lower latitudes (35°–55°), making them visible from the capital Khar-Vexar.
  6. Xha'Ruun bio-optical computers are resistant through optical pathways, with protected supporting electronics.
  7. The lower activity of Khar'Vex (K2V) partially compensates for the weak magnetosphere.
  8. Average magnetic field reversal: ~350,000 years, last — ~28,000 years ago.

Connections to other chapters: