Mid-infrared ultrashort high energy laser sources are opening up new opportunities in science, including keV-class high harmonic generation and monoenergetic MeV-class proton acceleration. As new higher energy sources become available, potential applications for atmospheric propagation can dramatically grow to include stand-off detection, laser communications, shock-driven remote terahertz enhancement and extended long-lived thermal waveguides to transport high power microwave and radiofrequency waves. We reveal a new paradigm for long-range, low-loss, ultrahigh power ultrashort pulse propagation at mid-infrared wavelengths in the atmosphere. Before the onset of critical self-focusing, energy in the fundamental wave continually leaks into shock-driven spectrally broadened higher harmonics. A persistent near-invariant solitonic leading edge on the multi-terawatt pulse waveform transports most of the power over hundredmetre-long distances. Such light bullets are resistant to uncontrolled multiple filamentation and are expected to spark extensive research in optics, where the use of mid-infrared lasers is currently much under-utilized. U ltrafast femtosecond laser pulses possess the unique property that they deliver extreme local fields, avoid avalanche ionization and yet deposit relatively little energy, thereby avoiding significant collateral damage. In the context of long-range atmospheric propagation of multi-terawatt femtosecond-duration laser pulses, the Ti:sapphire laser has been the standard workhorse and has promoted atmospheric studies ranging from femtosecond LIDAR 1 , remote laser-induced breakdown spectroscopy (LIBS) 2,3 , white light generation 4 , discharge triggering and guiding 5-7 , lightning control 8 and filament-induced water-cloud condensation in the free, sub-saturated atmosphere 9 .However, high accumulated plasmas, which tend to strongly defocus the pulse 10 , abruptly terminate propagation of individual filaments over sub-metre-long paths. Despite the remarkable swathe of applications that have been enabled with this ultraintense laser source, the ability to launch a super-intense intact electromagnetic pulse over long distances remains elusive. The reason for this has been understood for some time and is due to the tendency of a relatively wide 800 nm multi-terawatt beam to break up into tens or hundreds of light filaments with typical waists on the order of 100 µm, originally initiated via modulational instability 11,12 .The nucleation of filaments at 800 nm is typically random in space, and is also influenced by aberrations on the beam induced in the multiple-pass cascaded stages of the Ti:sapphire amplifiers. Much effort has been expended on attempts to control or elongate intense light filaments 13 , but with limited success primarily because each filament tends to die and reappear chaotically at different locations along the propagation path. Moreover, the light filaments tend to carry a power totalling on the order of 10-15% of the total power in the beam, leaving the remainder to ac...