SIMULATION LIVE

SOLAR LOOP SCREEN · ISOTHERMAL RESISTIVE 2.5D MHD

Search for life-like dynamics in a solar plasma.

A straightened coronal loop lets Alfvén and magnetosonic modes arise from positive density plus signed momentum and magnetic fields—then tests whether any organization escapes its driver.

12 τA TARGET0.00 τA elapsed

EMERGENCE STARTERS · NO GENOME SEEDED

Give the field a challenge, then let the dynamics decide.

INITIAL CARRIERW+ = W− = J = 0for every starter
strict emergence

Homogeneous coronal loop

Wave-supported magnetic organization

A uniform guide field and homogeneous coronal plasma begin with zero transverse velocity, zero magnetic perturbation and zero Elsässer carrier energy.

strict emergence

Fluctuation bath

Spontaneous individuation

No coherent body is inserted—only microscopic activity noise in a driven magnetized chamber.

morphology control

Fissioner alpha

Repeated body splitting

One unstructured bar of activity tests the classic grow–neck–split morphology.

strict emergence

Metastable propagule

Compositional inheritance

No body, shell or carrier is inserted. Microscopic activity noise drives two symmetric carrier populations and an emergent boundary proxy.

structure challenge

Loop challenge

Boundary maintenance

A hollow activity loop begins with no slow carrier and must either close, repair, transform, or dissolve.

structure challenge

Field filament

Transport-guided organization

A featureless narrow excitation tests whether anisotropic transport builds a persistent filament network.

ASSAY

Require bounded current structures to outlive drive cutoff, phase scrambling or detuning across several Alfvén crossing times.

FAIL IF

A candidate is locked to the footpoint driver, disappears under grid refinement, or fails matched no-drive and phase-scrambled controls.

ENGINEERED POSITIVE CONTROLS · EXCLUDED FROM EMERGENCE

Can these mechanics carry a glider-like plasma form at all?

Each launch writes only smooth density, momentum and magnetic source fields allowed by this solver, then turns the boundary driver off. An exact continuous state has probability zero, but every finite neighborhood of these controls is reachable under a full-support random initializer. Reachable does not mean probable.

EVIDENCE CLASSPOSITIVE CONTROLnever counted as spontaneous life
exact-wave analogue · seed 2,604,271

Alfvén packet glider

A smooth, one-direction Elsässer packet starts away from the boundary and should translate near the Alfvén speed before reflection.

Look for center-of-energy motion with translated-shape retention and no continuing footpoint input.
momentum-balanced wave · seed 2,451,903

Zero-net dipole glider

Two signed transverse lobes form one right-moving packet with approximately zero net transverse momentum.

Tests whether a less trivially biased localized packet can move coherently without a net kick.
topological memory control · seed 2,072,441

Flux-rope breather

A smooth magnetic-potential island, axial field core and matched circulating flow create a localized current-bearing structure.

Tests passive topology retention, oscillation and resistive decay; it is not expected to translate like a glider.
interaction control · seed 2,913,627

Counter-packet collision

Matched left- and right-moving Alfvén packets collide near the loop midpoint without boundary driving.

Tests whether interaction leaves a persistent localized remnant rather than two linearly passing waves.

96 × 58 REFERENCE PROBE · DRIVER OFFAlfvén packet passes through 0.75 τA (0.93 vA, 88% translated-shape match); the zero-net dipole passes through 0.50 τA, then falls below the energy threshold by 0.75 τA. The flux rope and symmetric collision do not pass the translation screen.

PERSISTENT EXPERIMENT RACK · NO AUTOMATIC RESET

Six chambers keep running while you inspect the main universe.

Matched arms share the same homogeneous state and driver coefficient stream; chamber B alone uses an independent forcing seed.

matched seed 1604271
Full solar MHD Areference
0.00 τA0 regionsm1 R² unresolvedP/τA unresolved
Full solar MHD Bindependent driver seed
0.00 τA0 regionsm1 R² unresolvedP/τA unresolved
Footpoint drive offformation null
0.00 τA0 regionsm1 R² unresolvedP/τA unresolved
Phase-scrambled drivesame modal power
0.00 τA0 regionsm1 R² unresolvedP/τA unresolved
Density-motion clampheuristic Alfvénic control
0.00 τA0 regionsm1 R² unresolvedP/τA unresolved
High dampingη×8 · ν×4
0.00 τA0 regionsm1 R² unresolvedP/τA unresolved

A standing wave can repeatedly cross the segmentation threshold without reproducing. Driver independence, cutoff survival and numerical convergence—not visual complexity—govern promotion.

PLASMA FIELD VIEW current + compression W+ / W− · current amber
MODEL SOLAR-LOOP · GRID 216×132
t* 0Δt≤ 0.120t/τA W±(0) = J(0) = 0driver vᵣₘₛ
0 coherent regionsthreshold Hc · lock · ∇·B
x*
y*

The homogeneous loop is ramping up its broadband footpoint driver. No plasma object or genome was inserted.

LINEAGE TRACE
provisional descent state-change candidate
Waiting for coherent attractors to cross the segmentation gate.

PERSISTENT TOP-K RECIPE ARCHIVE

The best recipes now survive refreshes and visitors.

Completed search generations are recorded globally. Community entries remain unverified and can never overwrite the paper’s reference results.

loading shared archive…
Run recipe search to scan chamber settings. Candidates are ranked only after a complete observation window.

Public archive ≠ verified evidence. Exact recipes are replayable, but promotion into the paper requires deterministic reruns, controls and a frozen model version.