phase fiasco eurorack modules

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Skalman

240dl

[i]

meteor shower

Skalman

The Skalman is a compact 8HP clock processor built on the Electrosmith Daisy Seed and programmed in C++ for precision timing and stability. It provides four independent clock channels, each capable of division or multiplication, making it a versatile tool for rhythmic modulation in Eurorack systems.

The module operates in two modes:

Internal Clock: Dial in a tempo directly with the Tempo knob.

External Clock: Feed an incoming gate signal via Clock In for synchronization with other modules.

Each of the four outputs can be set to a specific division or multiplication relative to the clock: /4, /3, /2, 1x, 2x, 3x, 4x. Channel parameters are adjusted via dedicated control knobs or externally modulated with CV inputs, enabling both precise configuration and dynamic performance control.

Key Features:

Four independent clock outputs (gate signals)

Selectable divisions and multiplications: /4, /3, /2, 1x, 2x, 3x, 4x

Internal or external clock operation

CV control per channel for modulation of division/multiplication

8HP width, streamlined interface, and low-latency DSP design

Skalman is designed as a straightforward, reliable clock utility that adapts easily to both sequencing and performance setups, giving you flexible rhythmic structures with minimal patching complexity.

240dl
Built on the powerful Daisy Seed platform, the 240 DL is a Eurorack distortion and FX module that takes inspiration from the legendary Volvo 240, a Swedish icon of durability, grit, and no-nonsense character. Just like the car, this module isn’t about polish — it’s about raw personality, stubborn reliability, and a touch of Nordic eccentricity.

The 240 DL is a Eurorack multi-effect distortion module built on the Electrosmith Daisy Seed platform and developed in C++ for optimized performance and stability. It doesn’t just add distortion. It gives your signal the attitude of a roaring old-school machine built for endless miles.

Its processing chain combines compression, modal filtering, overdrive, sample reduction, bitcrushing, notch filtering, and reverb, giving a wide spectrum of sound shaping — from subtle harmonic enhancement to highly degraded, textural distortion. Each stage is internally routable, allowing for complex interaction between dynamic control, filtering, and time-based effects.

Key design considerations include:

Precision DSP coding for consistent results and low latency.

Internal modulation paths enabling dynamic control without external CV.

Stereo signal flow with additional noise sources (white and dust) for expanded timbral possibilities.

Configurable routing for both subtle processing and aggressive signal destruction.

[i]

The [i] is a 8HP Eurorack CV controller built on the Electrosmith Daisy Seed and programmed in C++ for precision and low-latency performance. It combines tactile control with musical intelligence, making it a versatile source of melodic or modulation CV.

At its core is a 12-point capacitive touch strip, allowing direct finger interaction to set pitch or CV values. Each touch position corresponds to a note or voltage step, with a clear LED display showing the active point in real time.

The module offers flexible output modes via the Scale knob:

Off (free CV mode): Outputs raw CV proportional to touch position.

Chromatic: Quantized to semitones across the octave.

Major / Minor: Quantized to diatonic scales, with Root Key selection via dedicated knob.

To shape the output response, the Attack and Decay knobs provide slew limiting, transforming abrupt changes into expressive glides or envelopes.

Key Features:

12-point capacitive touch controller with LED feedback

Selectable output modes: CV, Chromatic, Major, Minor

Root key selection for scale quantization

Attack and Decay controls for slew/glide shaping

Switchable CV or 1V/Oct output for melodic integration'

Compact 8HP format

The [i] bridges performance and control, functioning equally well as a melodic controller, modulation source, or experimental gesture interface.

meteor shower

Meteor showers are astronomical events during which numerous meteors become visible as Earth passes through a stream of cosmic debris. These meteors are caused by small particles, often no larger than grains of sand, entering Earth's atmosphere at very high velocities, typically between 11 and 72 kilometers per second. As they collide with atmospheric molecules, the resulting friction heats them up, causing them to glow brightly and produce the visible streaks of light commonly known as "shooting stars." Despite the name, these meteors are unrelated to actual stars.

Meteors within a shower appear to originate from a specific point in the night sky, known as the radiant. This effect is caused by perspective. Although the meteoroids are traveling in nearly parallel paths, they appear to diverge from a single location due to the observer's viewpoint on Earth. Meteor showers are typically named after the constellation in which this radiant is located. For example, the Perseids have a radiant in the constellation Perseus, and the Geminids appear to radiate from Gemini.

Meteor showers occur at consistent times each year because Earth encounters the same streams of debris at fixed points in its orbit around the Sun. These debris streams are remnants of comets or, in some cases, asteroids that have left behind particulate trails during their passages through the inner solar system. As Earth intersects these trails, particles from the parent body enter the atmosphere and produce the meteor shower. Well-known showers like the Perseids in mid-August and the Geminids in mid-December are particularly active and have been observed and recorded for centuries.

The majority of meteor showers originate from comets, which are icy bodies composed of rock, dust, and frozen gases. When a comet approaches the Sun, it begins to sublimate, releasing material that becomes distributed along its orbital path. Over time, this material forms a meteoroid stream. When Earth crosses one of these streams, a meteor shower becomes visible. Some showers, such as the Geminids, are associated with asteroids. A notable example is asteroid 3200 Phaethon, which behaves somewhat like a comet and may be a "rock comet" or a fragment of a previously active body. The exact nature of such parent objects remains an active area of research.

Most meteoroids are too small to survive their fiery passage through the atmosphere and are entirely vaporized at altitudes ranging from 80 to 120 kilometers. However, in rare cases, larger fragments may endure the intense heat and pressure, reaching the ground as meteorites. Such events are uncommon during typical meteor showers, since the particles involved are generally small and fragile.

Meteor showers have long fascinated humanity. In antiquity, they were often interpreted as omens or supernatural signs. Today, they are appreciated both for their visual spectacle and their scientific value. By studying meteor showers and the composition of meteoroids, astronomers gain insights into the nature of comets, asteroids, and the early solar system. Observing a meteor shower is also a vivid reminder of Earth's motion through space and its ongoing interaction with the broader solar environment. Even with a full understanding of the physics involved, the sight of meteors tracing brilliant paths across the night sky continues to evoke a sense of wonder and curiosity.